Liste von Doppel- und Mehrfachsternen
aus Wikipedia, der freien Enzyklopädie
Diese Liste von Doppel- und Mehrfachsternen enthält die meisten visuellen Doppel- und Mehrfachsterne mit Bayer- und Flamsteed-Bezeichnung. Darüber hinaus sind enthalten:
- einige Doppelsterne der 5. und 6. Größenklasse ohne Bayer- und Flamsteed-Bezeichnung mit etwa gleichen Helligkeiten,
- besonders sonnennahe Systeme (bis ca. 20 Lj),
- einige astrophysikalisch interessante Systeme.
Die Liste enthält in der Regel nicht:
- Doppel- und Mehrfachsterne, deren Begleiter nur schwache, unverbundene Feldsterne sind,
- nicht aufgelöste spektroskopische Doppelsterne (außer Untersysteme eines visuellen Doppelsterns),
- unsichere und unbestätigte Komponenten,
- Röntgendoppelsterne.
Braune Zwerge werden in der Liste wie Sterne behandelt.
Erläuterung der Liste
- Stb. – Sternbild (lateinisches Kürzel), in dem das System liegt.
- System – Bezeichnung des Systems. Innerhalb eines Sternbildes kommen zuerst alle Systeme mit Bayer-Bezeichnung, danach alle Systeme mit Flamsteed-Bezeichnung, danach alle sonstigen Systeme.
- Untersystem (nur bei Mehrfachsternen) – Die Zahl gibt die hierarchische Ebene an (1 = Hauptsystem, 2 = Untersystem, 3 = Unter-Untersystem usw.). In Klammer steht die Bezeichnung des Hauptsterns (Hauptkomponente, engl. primary) und des Begleitsterns (Begleiter, engl. secondary), getrennt durch einen Schrägstrich. Die Bezeichnung richtet sich nach dem WDS bzw. dem allgemeinen Benennungsschema bei Mehrfachsternen (Hartkopf & Mason 2004, bibcode:2004RMxAC..21...83H).
- Typ – Einteilung nach Beobachtbarkeit. Abgesehen von den optischen Doppelsternen (O), die nur zufällig am Himmel nebeneinander stehen, unterscheidet man bei den physischen (d. h. gravitativ aneinander gebundenen) Doppelsternen zwischen visuellen, spektroskopischen, astrometrischen und fotometrischen (bedeckungsveränderlichen) Doppelsternen. Die Typen schließen sich gegenseitig nicht aus, z. B. konnten viele spektroskopisch oder astrometrisch entdeckte Doppelsterne später mit besserer Teleskoptechnik in visuelle Doppelsterne aufgelöst werden. Der Übergang zwischen „klassischen“ visuellen Doppelsternen und CPM-Paaren ist unscharf.
- Visuelle Doppelsterne (engl. visual binaries) sind Doppelsterne, die in zwei getrennte Lichtquellen aufgelöst werden können. V – „klassischer“ visueller Doppelstern, der mit dem Auge (mit Hilfe eines Fernrohrs) trennbar ist oder es zum Zeitpunkt der Entdeckung war. V(aO) – konnte mit aktiver oder adaptiver Optik aufgelöst werden. V(IR) – konnte im infraroten Bereich des elektromagnetischen Spektrums aufgelöst werden. V(HST) – konnte mit dem Hubble-Weltraumteleskop aufgelöst werden. I – mit Long-Baseline-Interferometrie auflösbar. SI – mit Speckle-Interferometrie auflösbar. CPM – common proper motion pairs sind weite visuelle Doppelsterne, die ihre Verwandtschaft durch ihre gemeinsame Eigenbewegung verraten. Sie zeigen kaum bis keine Relativbewegung zueinander und sind nur schwach bis gar nicht aneinander gebunden. Ein gemeinsamer Entstehungsursprung (Sternhaufen, Assoziation) wird angenommen.
- SB – Spektroskopische Doppelsterne (engl. spectroscopic binaries) weisen periodische Verschiebungen bzw. Aufspaltungen der Spektrallinien aufgrund der sich ändernden Radialgeschwindigkeit durch den Umlauf auf (siehe: Doppler-Effekt).
- A – Astrometrische Doppelsterne (engl. astrometric binaries) verraten sich durch ihre nichtlineare Eigenbewegung aufgrund des Umlaufs um das Baryzentrum mit ihrer nicht sichtbaren Komponente. Anmerkung: Oft wurden enge visuelle (interferometrische) Doppelsterne astrometrisch entdeckt. Der Einfachheit halber wird der Typ der astrometrischen Doppelsterne zusätzlich nur bei nicht-visuellen Systemen (SB, E) angeführt.
- E – Fotometrische (bedeckungsveränderliche) Doppelsterne (engl. eclipsing binaries) zeigen periodische Helligkeitsabfälle infolge der gegenseitigen Bedeckungen der Komponenten.
- Neben diesen Grundtypen gibt es noch weitere Kategorien, die aber in der Liste nicht verwendet werden, z. B. durch Sternbedeckungen nachgewiesene Doppelsterne (engl. occultation binaries), Röntgendoppelsterne (engl. X-ray binaries), so genannte Composite-Spectra-Sterne (roter Riese + A/B-Hauptreihenstern) etc.
- V1, V2 – Scheinbare visuelle Helligkeit der Hauptkomponente (V1) und des Begleiters (V2). Bei nicht aufgelösten Systemen ist die Helligkeit des Begleiters in der Regel unbekannt; in diesem Fall ist die Helligkeit in V1 die Gesamthelligkeit beider Komponenten (auf einen Zellenverbund wurde verzichtet).
- ρ – Winkeldistanz zwischen den Komponenten (entfällt bei spektroskopischen und interferometrischen Doppelsternen).
- Ep. – Jahr, in dem die Winkeldistanz gemessen wurde (entfällt bei spektroskopischen und interferometrischen Doppelsternen).
- U – Umlaufzeit in Jahren (a) oder Tagen (d). Die Umlaufzeit ist ohne Fehlerangabe und gerundet angegeben. Sie ist grün markiert, wenn die Qualität der Bahnelemente im 6th Orbit Catalog mit Grade 1 („endgültig“) oder 2 („gut“) bewertet ist, d. h. künftig keine großen Anpassungen der Bahnelemente mehr zu erwarten sind.
- S1, S2 – Spektralklasse der Hauptkomponente (S1) und des Begleiters (S2). Ein angehängter Doppelpunkt (z. B. K3:) zeigt an, dass der Spektraltyp unsicher ist.
- M1, M2 – Masse der Hauptkomponente (M1) und des Begleiters (M2) in Sonnenmassen. Ein Σ zeigt an, dass sich die Masse aus mehreren Einzelsternen zusammensetzt.
- Entdeckercode – Details siehe Artikelende.
- WDS – Nummer im Washington Double Star Catalog. Die WDS-Nummer fungiert zugleich als Koordinatenangabe, z. B. WDS 09285+0903 entspricht RA = 09 h 28,5 min, Dec = 09° 03'.
- d – Entfernung des Systems in Parsec. Fett markierte Entfernungen stammen von präzise bestimmten dynamischen Parallaxen. Bei optischen Doppelsternen bezieht sich die Entfernung auf die hellere Komponente.
- Quelle – Details siehe Artikelende.
Liste
Die Spalten sind mit einem Klick auf den Doppelpfeil sortierbar.
Stb. | System | Untersystem | Typ | V1 | V2 | ρ | Ep. | U | S1 | S2 | M1 | M2 | Entdecker- code |
WDS | d | Quelle |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
And | α And (Sirrah) | I/SB | 2,2 | 4,2 | – | – | 96,7 d | B8 IV–VHgMn | 3,8 ± 0,2 | 1,6 ± 0,1 | MKT 11 | 00084+2905 | 30 | [1] (M, d) | ||
And | γ And | 1 (γ1 = A / γ2 = BC) | V | 2,3 | 5,0 | 9,8″ | 2020 | K2 IIb | B9 V + A3 V + A0 V | Σ 8,3 ± 0,3 | STF 205 | 02039+4220 | 120 | [2] (SBa/Bb, M), [3] (UBa/Bb) | ||
2 (B/C) | V | 5,3 | 6,5 | 0,2″ | 2010 | 63 a | B9 V + A3 V | A0 V | Σ 5,7 | 2,6 | STT 38 | |||||
3 (Ba/Bb) | SB | 6,5 | . | – | – | 2,67 d | B9 V | A3 V | 3,3 | 2,4 | ||||||
And | δ And | V(aO)/SB | 3,3 | 10,0 | 0,4″ | 2014 | 53 a | K3 III | K4 | Σ 2,6 ± 0,4 | BTM 1 | 00393+3052 | 32 | [4] (S, M) | ||
And | η And | I/SB | 4,4 | . | – | – | 116 d | G8 III | G8 III | 2,4 | 2,3 | MKT 2 | 00572+2325 | 70 | [5] (S, M) | |
And | ο And | 1 (A/B) | SI | 3,7 | 6,0 | 0,2″ | 2015 | 117 a | B6 IIIpe + A2p | Σ 18 ± 2 | WRH 37 | 23019+4220 | 210 | [6] (UBa/Bb), [3] (SAa/Ab), [7] (M) | ||
2 (Aa/Ab) | SI | 3,8 | 5,7 | 0,1″ | 1997 | 5,6 a | B6 IIIpe | A2p | BLA 12 | |||||||
2 (Ba/Bb) | SB | 6,0 | . | – | – | 33,0 d | ||||||||||
And | π And | 1 (A/B) | CPM | 4,4 | 7,1 | 36,2″ | 2019 | B3 V + B6 V | A6 V | Σ 10,6 | H 5 17 | 00369+3343 | 180 | [8] (SAa/Ab, M) | ||
2 (Aa/Ab) | I/SB | 4,9 | 5,3 | – | – | 144 d | B3 V | B6 V | 5,8 | 4,8 | MKT 1 | |||||
And | φ And | V | 4,6 | 5,6 | 0,6″ | 2016 | 550 a | B6 IV | B9 V | Σ 6,5 ± 2,8 | STT 515 | 01095+4715 | 220 | [9] (S, M) | ||
And | ψ And | 1 (Aa,Ab/Ac) | SI | 5,2 | 8,1 | 0,4″ | 2018 | MCA 75 | 23460+4625 | 310 | ||||||
2 (Aa/Ab) | SI | 5,2 | . | 0,2″ | 2003 | MCA 75 | ||||||||||
And | ω And | 1 (A/B) | V | 4,8 | 11,7 | 0,7″ | 2002 | F3 V + F5 V | Σ 1,9 | BU 999 | 01277+4524 | 29 | [10] (S, M) | |||
2 (Aa/Ab) | I/SB | 4,8 | . | – | – | 255 d | F3 V | F5 V | 1,0 | 0,9 | CIA 4 | |||||
And | 2 And | V | 5,2 | 7,7 | 0,2″ | 2009 | 74 a | B8 | A7 | 3,3 | 1,9 | BU 1147 | 23026+4245 | 130 | [11] (S, M) | |
And | 26 And | V | 6,1 | 10,1 | 6,1″ | 2016 | STT 5 | 00187+4347 | 190 | |||||||
And | 36 And | V | 6,1 | 6,5 | 1,2″ | 2019 | 168 a | G6 IV | K6 IV | Σ 1,9 ± 0,2 | STF 73 | 00550+2338 | 38 | [9] (S, M) | ||
And | 56 And | O | 5,8 | 6,1 | 202,5″ | 2014 | STFA 4 | 01562+3715 | 100 | |||||||
And | 59 And | V | 6,1 | 6,7 | 16,6″ | 2019 | STF 222 | 02109+3902 | 140 | |||||||
And | HR 647 | V | 6,6 | 7,2 | 0,7″ | 2018 | 145 a | F2 | F7 | Σ 2,4 ± 0,3 | STF 228 | 02140+4729 | 40 | [12] (S, M) | ||
And | HR 283 | V | 6,0 | 6,8 | 7,9″ | 2018 | 9200 a | B9,5 Vnn | A2 Vn | STF 79 | 01001+4443 | 150 | ||||
And | HR 9074 | V | 6,5 | 6,7 | 2,5″ | 2019 | 570 a | G0 V | G0 V | STF 3050 | 23595+3343 | 30 | [13] (S) | |||
And | Groombridge 34 | V | 8,3 | 11,4 | 34,1″ | 2019 | 2600 a | M1 V | M3,5 V | 0,4 | 0,2 | GRB 34 | 00184+4401 | 3,6 | [14] (S1, M1), [15] (S2, M2) | |
Ant | δ Ant | V | 5,6 | 9,8 | 10,3″ | 2017 | B9–9,5 V | F9 Ve | H N 50 | 10296-3036 | 140 | |||||
Ant | ζ1 Ant | V | 6,2 | 6,8 | 8,3″ | 2020 | A1 V | A1 V | DUN 78 | 09308-3153 | 120 | |||||
Ant | θ Ant | SI | 5,3 | 6,2 | 0,0″ | 2020 | 18,3 a | G7 III | A8 V | 2,1 ± 0,5 | 1,8 ± 0,1 | FIN 326 | 09442-2746 | 100 | [16] (S, M) | |
Ant | 2MASS 0939-2448 | . | . | – | – | T8 | 0,03–0,05 | 0,02–0,03 | 5,3 | [17] (S, M, d) | ||||||
Aps | δ1 Aps | CPM | 4,9 | 5,4 | 103,0″ | 2010 | BSO 22 | 16203-7842 | 230 | |||||||
Aps | ι Aps | SI | 5,9 | 6,5 | 0,1″ | 2018 | 160 a | B9 | B9,5 | 5,4 | 4,7 | FIN 373 | 17221-7007 | 320 | [11] (S, M) | |
Aql | β Aql | V | 3,8 | 11,4 | 13,4″ | 2015 | G8 IV | M3 | STT 532 | 19553+0624 | 14 | |||||
Aql | δ Aql | SI/SB | 3,4 | 9,2 | 0,1″ | 1979 | 3,4 a | F0 IV | K: | ≈ 1,7 | ≈ 0,7 | BNU 6 | 19255+0307 | 16 | [18] (V2, S, M) | |
Aql | ε Aql | SB/A | 4,0 | . | – | – | 3,5 a | eps Aql | 18596+1504 | 42 | ||||||
Aql | η Aql | V(HST) | 3,8 | 10,0 | 0,7″ | 2012 | ≈ 870 a | F6 Iab | B9,8 V | 5,7 | 2,3 | EVS 2 | 19525+0100 | 270 | [19] (U, M, d) | |
Aql | θ Aql | I/SB | 3,5 | 5,0 | – | – | 17,1 d | B9 III | B9 III | 3,2 ± 0,7 | 2,5 ± 0,6 | MKT 10 | 20113-0049 | 71 | [3] (S), [1] (M, d) | |
Aql | π Aql | V | 6,3 | 6,8 | 1,4″ | 2019 | G8 III | A3 V | STF 2583 | 19487+1149 | 160 | |||||
Aql | χ Aql | V | 5,4 | 6,6 | 0,4″ | 2020 | STT 380 | 19426+1150 | 260 | |||||||
Aql | 5 Aql | 1 (A/B) | V | 5,9 | 7,0 | 12,5″ | 2019 | kA3hA5VmA6 | kA4hF0VmF3 | STF 2379 | 18465-0058 | 94 | [20] (SAa/Ab), [3] (UAa od. Ab) | |||
2 (Aa/Ab) | SI | 5,9 | 6,8 | 0,0″ | 2014 | 41 a | Am | Am | MCA 53 | |||||||
3 (Aa oder Ab) | SB | . | . | – | – | 4,77 d | Am | |||||||||
Aql | 11 Aql | O | 5,3 | 9,3 | 20,8″ | 2019 | STF 2424 | 18591+1338 | 48 | |||||||
Aql | 15 Aql | O | 5,5 | 7,0 | 39,6″ | 2019 | SHJ 286 | 19050-0402 | 95 | |||||||
Aql | 18 Aql | V | 5,4 | 6,4 | 0,3″ | 2015 | 210 a | HEI 568 | 19070+1104 | 210 | ||||||
Aql | 23 Aql | V | 5,3 | 8,3 | 3,2″ | 2011 | STF 2492 | 19185+0105 | 120 | |||||||
Aql | 45 Aql | SI | 5,9 | 7,6 | 0,1″ | 2020 | 10,2 a | A3 IV | CHR 88 | 19407-0037 | 110 | |||||
Aql | 57 Aql | CPM | 5,7 | 6,4 | 36,3″ | 2019 | B7 Vn | B8 V | STF 2594 | 19546-0814 | 140 | |||||
Aql | QS Aql | 1 (A/B) | V | 6,7 | 6,8 | 0,1″ | 2018 | 77 a | B5 V + F3 | B4 | KUI 93 | 19411+1349 | 680 | [21] (UAa/Ab, S) | ||
2 (Aa/Ab) | E/SB | 6,7 | . | – | – | 2,51 d | B5 V | F3 | ||||||||
Aql | Gliese 752 / VB 10 | CPM | 9,1 | 17,4 | 75,8″ | 2012 | dM3,5 | M8 Ve | 0,5 | 0,09 | LDS 6334 | 19169+0510 | 5,9 | [22] (S, M) | ||
Aqr | δ Aqr | I/A | 3,3 | . | – | – | 1,3 a | A3 V | G5: | 76 Aqr | 22547-1549 | 35 | [23] (S) | |||
Aqr | ζ Aqr | 1 (ζ2 = A / ζ1 = B) | V | 4,3 | 4,5 | 2,4″ | 2020 | 430 a | F1 IV | F3 IV | Σ 2,0 | 1,4 | STF 2909 | 22288-0001 | 28 | [24] (S), [25] (M) |
2 (Aa/Ab) | SI | 4,3 | 11,3 | 0,7″ | 2020 | 25,1 a | F1 IV | 1,4 | 0,6 | EBE 1 | ||||||
Aqr | ξ Aqr | SI/SB | 4,8 | 7,0 | 0,0″ | 2008 | 25,5 a | MCA 68 | 21378-0751 | 55 | ||||||
Aqr | ψ1 Aqr | 1 (A/BC) | CPM | 4,4 | 9,9 | 48,9″ | 2014 | K1 III | K1–2 V | 1,4 ± 0,3 | STFB 12 | 23159-0905 | 44 | [26] (M) | ||
2 (B/C) | V | 10,5 | 10,7 | 0,4″ | 2020 | 84 a | K1–2 V | BU 1220 | ||||||||
Aqr | ψ3 Aqr | V | 5,0 | 9,0 | 1,5″ | 2015 | HO 199 | 23190-0937 | 73 | |||||||
Aqr | ω2 Aqr | V | 4,5 | 9,9 | 5,5″ | 2012 | BU 279 | 23427-1433 | 46 | |||||||
Aqr | 4 Aqr | V | 6,4 | 7,4 | 0,7″ | 2020 | 200 a | F7 IV | F6: V: | 1,6 | 1,3 | STF 2729 | 20514-0538 | 61 | [27] (M) | |
Aqr | 12 Aqr | 1 (A/B) | V | 5,8 | 7,5 | 2,5″ | 2017 | STF 2745 | 21041-0549 | 150 | ||||||
2 (Aa/Ab) | SI | 5,9 | 8,3 | 0,3″ | 2017 | MCA 66 | ||||||||||
Aqr | 24 Aqr | 1 (A/B) | V | 6,9 | 8,4 | 0,0″ | 2020 | 48,7 a | BU 1212 | 21395-0003 | 40 | [3] (UAa/Ab) | ||||
2 (Aa/Ab) | SB | 6,9 | . | – | – | 5,88 d | ||||||||||
Aqr | 29 Aqr | 1 (A/B) | V | 7,2 | 7,2 | 3,8″ | 2016 | A2 V + K0 III | G0 II | S 802 | 22024-1658 | 180 | [21] (UAa/Ab, SAa/Ab) | |||
2 (Aa/Ab) | E/SB | 7,2 | . | – | – | 0,95 d | A2 V | K0 III | ||||||||
Aqr | 41 Aqr | V | 5,6 | 6,7 | 5,2″ | 2015 | K0 III | F2 V | H N 56 | 22143-2104 | 72 | |||||
Aqr | 51 Aqr | V | 6,5 | 6,6 | 0,5″ | 2019 | 145 a | A1 | A1 | 2,5 | 2,4 | BU 172 | 22241-0450 | 120 | [11] (S, M) | |
Aqr | 53 Aqr | 1 (A/B) | V | 6,3 | 6,4 | 1,2″ | 2019 | 2000 a | G2 V | G3 V | SHJ 345 | 22266-1645 | 19 | [3] (UBa/Bb) | ||
2 (Ba/Bb) | SB | 6,4 | . | – | – | 257 d | G2 V | |||||||||
Aqr | 74 Aqr | 1 (A/B) | SI | 5,8 | 6,4 | 0,1″ | 2020 | 9,5 a | B9p | B | Σ ≈ 15 | MCA 73 | 22535-1137 | 170 | [3] (UAa/Ab), [28] (S, M) | |
2 (Aa/Ab) | SB | 5,8 | . | – | – | 3,43 d | B9p | |||||||||
Aqr | 83 Aqr | V | 6,2 | 6,3 | 0,2″ | 2018 | 21,8 a | F2 V | F2 V | A 417 | 23052-0742 | 64 | [24] (S) | |||
Aqr | 86 Aqr | SI | 4,8 | 6,8 | 0,2″ | 2020 | HDS 3293 | 23067-2345 | 56 | |||||||
Aqr | 89 Aqr | V | 5,3 | 6,0 | 0,2″ | 2018 | 108 a | G2 III | A2 V | RST 3320 | 23099-2227 | 150 | ||||
Aqr | 94 Aqr | 1 (A/B) | V | 5,2 | 7,0 | 12,1″ | 2018 | G5–8 IV + K2–3 | K2 | Σ 1,9 | STF 2998 | 23191-1328 | 22 | [29] (S, M) | ||
2 (Aa/Ab) | SI/SB | 5,2 | 6,7 | 0,2″ | 2020 | 6,3 a | G5–8 IV | K2–3 | 1,1 | 0,8 | MCA 74 | |||||
Aqr | 97 Aqr | V | 5,6 | 6,7 | 0,1″ | 2020 | 64 a | A3 | A8 | 2,0–3,7 | 1,6 | HU 295 | 23227-1502 | 65 | [11] (S, M) | |
Aqr | 101 Aqr | V | 4,8 | 7,7 | 1,0″ | 2009 | B 1900 | 23333-2055 | 90 | |||||||
Aqr | 107 Aqr | V | 5,7 | 6,5 | 7,0″ | 2018 | A9 IV | F2 V | H 2 24 | 23460-1841 | 62 | |||||
Aqr | R Aqr | V(aO)/SB | 7,7 | . | – | – | 44 a | M6,5–8,5e | D: | 1,0–1,5 | 0,6–1,0 | 320 | [30] (V), [31] (U, S2, M) | |||
Aqr | EZ Aqr | 1 (AC/B) | SI/SB | 12,2 | 12,9 | 0,1″ | 2020 | 2,3 a | M4 V + M | M | Σ 0,22 | 0,12 | BLA 10 | 22385-1519 | 3,4 | [32] (S, M) |
2 (A/C) | SB | 12,2 | . | – | – | 3,79 d | M4 V | M | 0,12 | 0,10 | Gl 866 | |||||
Ara | γ Ara | CPM | 3,3 | 10,2 | 18,4″ | 2016 | HJ 4942 | 17254-5623 | 340 | |||||||
Ara | δ Ara | A | 3,6 | . | – | – | 2,9 a | del Ara | 17311-6041 | 61 | ||||||
Ara | ε2 Ara | 1 (A/C) | CPM | 5,4 | 13,5 | 113,6″ | 2015 | F5 VFe | DA3,2 | SKF 103 | 17031-5314 | 26 | ||||
2 (Aa/Ab) | SI | 5,4 | 8,7 | 0,7″ | 2020 | 41 a | F5 VFe | HDS 2412 | ||||||||
Ara | ν1 Ara (V539 Ara) | 1 (A/B) | V | 5,7 | 9,2 | 12,3″ | 2016 | B3 V + B4 V | A0–1 V | Σ 11,5 | HJ 4978 | 17505-5337 | 360 | [21] (U, S), [33] (M, d) | ||
2 (Aa/Ab) | E/SB | 5,7 | . | – | – | 3,17 d | B3 V | B4 V | 6,2 | 5,3 | ||||||
Ara | 41 Ara | V | 5,6 | 8,9 | 10,6″ | 2019 | 610 a | G9 V | M0 VpCaCr | BSO 13 | 17191-4638 | 8,8 | ||||
Ara | R Ara | 1 (A/B) | V | 7,2 | 7,8 | 3,7″ | 2016 | B5 V + F1 IV | Σ 6,5 | HJ 4866 | 16397-5700 | 120 | [34] (UAa/Ab, S, M) | |||
2 (Aa/Ab) | E/SB | 7,2 | . | – | – | 4,43 d | B5 V | F1 IV | 5 | 1,5 | ||||||
Ara | HR 6477 | 1 (AB/C) | CPM | 5,2 | 7,1 | 102,5″ | 2016 | B8 V + B9 V | B9,5 V | DUN 216 | 17269-4551 | 190 | ||||
2 (A/B) | V | 5,6 | 6,5 | 2,1″ | 2016 | B8 V | B9 V | HJ 4949 | ||||||||
Ari | β Ari | I/SB | 2,6 | 5,2 | – | – | 107 d | A5 V | 2,0 | 1,0 | MKT 3 | 01546+2049 | 18 | [1] (S, M, d) | ||
Ari | γ Ari | V | 4,5 | 4,6 | 7,4″ | 2020 | A2 IVpSiSrCr | A0 Vnp | STF 180 | 01535+1918 | 50 | |||||
Ari | ε Ari | V | 5,2 | 5,6 | 1,5″ | 2019 | 710 a | A2 IV | A3 IVs | STF 333 | 02592+2120 | 100 | ||||
Ari | λ Ari | CPM | 4,8 | 6,7 | 37,3″ | 2019 | H 5 12 | 01579+2336 | 39 | |||||||
Ari | μ Ari | SI | 5,7 | 6,2 | 0,0″ | 2020 | 8,8 a | A1 V | F2 V | 3,4 ± 1,7 | 2,1 ± 1,7 | BLA 1 | 02424+2001 | 140 | [35] (S, M) | |
Ari | π Ari | V | 5,3 | 8,0 | 3,3″ | 2015 | STF 311 | 02493+1728 | 240 | |||||||
Ari | τ1 Ari | V | 5,3 | 8,1 | 0,9″ | 2016 | COU 259 | 03212+2109 | 160 | |||||||
Ari | 1 Ari | V | 6,3 | 7,2 | 2,9″ | 2018 | K1 III | A6 V | STF 174 | 01501+2217 | 180 | [13] (S) | ||||
Ari | 10 Ari | V | 5,8 | 7,9 | 1,3″ | 2018 | 330 a | F8 IV | F9 V | STF 208 | 02037+2556 | 49 | [24] (S) | |||
Ari | 21 Ari | V | 6,4 | 6,5 | 0,2″ | 2014 | 23,6 a | F5 V | F5 V | 1,4 | 1,4 | COU 79 | 02157+2503 | 51 | [36] (S, M) | |
Ari | 30 Ari | 1 (A/BC) | CPM | 6,5 | 7,0 | 37,9″ | 2019 | F5 V | F8 V + M1 V | Σ 1,6 | STFA 5 | 02370+2439 | 45 | [3] (UAa/Ab), [37] (SB/C, MB/C) | ||
2 (Aa/Ab) | SB | 6,5 | . | – | – | 1,11 d | F5 V | |||||||||
2 (B/C) | V(aO) | 7,0 | 11,0 | 0,6″ | 2018 | F8 V | M1 V | 1,1 | 0,5 | RAO 8 | ||||||
Ari | 31 Ari | SI | 5,7 | 5,8 | 0,0″ | 2020 | 3,8 a | F7 V | F7 V | Σ 3,4 | MCA 7 | 02366+1227 | 35 | [38] (S, M) | ||
Ari | 52 Ari | 1 (AB/C) | V | 5,5 | 10,8 | 5,1″ | 2005 | B9 + B9 | Σ 7,2 | STF 346 | 03054+2515 | 170 | [11] (S, M) | |||
2 (A/B) | V | 6,2 | 6,2 | 0,5″ | 2016 | 230 a | B9 | B9 | 3,6 | 3,6 | STF 346 | |||||
Ari | 63 Ari | SI | 5,3 | 8,1 | 0,3″ | 2012 | HDS 423 | 03228+2045 | 97 | |||||||
Ari | 66 Ari | 1 (A/B) | V | 6,2 | 10,5 | 0,7″ | 2018 | BU 878 | 03284+2248 | 71 | ||||||
2 (Aa/Ab) | SI | 6,0 | 7,4 | 0,1″ | 2008 | BAG 2 | ||||||||||
Aur | α Aur (Capella) | 1 (A/HL) | CPM | 0,1 | 10,0 | 722,8″ | 2013 | G8 III + G0 III | M2 + M4: | Σ 5,1 | Σ 1,1 | FRH 1 | 05167+4600 | 13,2 | [39] (VAa/Ab, UH/L, SAa/Ab, M, d), [40] (SH/L) | |
2 (Aa/Ab) | I/SB | 0,9 | 0,8 | – | – | 104 d | G8 III | G0 III | 2,6 | 2,5 | ANJ 1 | |||||
2 (H/L) | V | 10,0 | 13,5 | 3,5″ | 2015 | ≈ 300 a | M2 | M4: | 0,6 | 0,5 | ST 3 | |||||
Aur | β Aur (Menkalinan) | E/I/SB | 3,3 | 3,5 | – | – | 3,96 d | A1m | A1m | 2,4 | 2,3 | KOE 1 | 05595+4457 | 25 | [33] (S, M) | |
Aur | ε Aur (Almaaz) | E/SB/A | 3,0 | . | – | – | 27,1 a | F0 Ia | ≈ 2 vs. 15 | ≈ 6 vs. 14 | eps Aur | 05020+4349 | 1500 | [41][42] (S, M), [43] (d) | ||
Aur | ζ Aur | E/I/SB | 3,8 | . | – | – | 2,7 a | K4 Ib | B6 V | 5,6 | 4,7 | MKT 6 | 05025+4105 | 240 | [5] (S, M) | |
Aur | θ Aur | V | 2,6 | 7,2 | 4,2″ | 2019 | 470 a | B9 IV | G2 V | STT 545 | 05597+3713 | 51 | [24] (S) | |||
Aur | ψ5 Aur | O | 5,3 | 8,7 | 29,4″ | 2013 | SHJ 75 | 06467+4335 | 17 | |||||||
Aur | ω Aur | V | 5,0 | 8,2 | 4,7″ | 2019 | A1 V | F9 | STF 616 | 04593+3753 | 50 | |||||
Aur | 5 Aur | 1 (A/B) | V | 6,0 | 9,5 | 4,1″ | 2017 | 1600 a | F5 V | 1,4 | 0,9 | STT 92 | 05003+3924 | 57 | [44] (M) | |
2 (Aa/Ab) | SI | 6,0 | . | 0,1″ | 2018 | F5 V | CHR 159 | |||||||||
Aur | 14 Aur | 1 (A/C) | V | 5,0 | 7,3 | 14,3″ | 2019 | A9 V | F2 V + DA1,3 | STF 653 | 05154+3241 | 82 | [3] (UAa/Ab, UCa1/Ca2), [45] (UCa/Cb), [46] (SCa/Cb) | |||
2 (Aa/Ab) | SB | 5,0 | . | – | – | 3,79 d | A9 V | |||||||||
2 (Ca/Cb) | V(HST) | 7,3 | 14,1 | 2,0″ | 1999 | ≈ 1300 a | F2 V | DA1,3 | BAS 5 | |||||||
3 (Ca1/Ca2) | SB | 7,3 | . | – | – | 2,99 d | F2 V | |||||||||
Aur | 16 Aur | 1 (A/B) | V | 4,8 | 10,6 | 4,1″ | 2002 | STT 103 | 05182+3322 | 71 | ||||||
2 (Aa/Ab) | SB/A | 4,8 | . | – | – | 1,2 a | ||||||||||
Aur | 26 Aur | 1 (AB/C) | V | 5,5 | 8,4 | 12,4″ | 2019 | ≈ 46 000 a | G8 III + B9,5 V | A6 V | Σ 5,1 ± 1,4 | 2,1 | STF 753 | 05386+3030 | 170 | [47] (UAB/C, S, M) |
1 (A/B) | V | 6,3 | 6,2 | 0,2″ | 2010 | 53 a | G8 III | B9,5 V | 2,1 ± 1,0 | 3,0 ± 0,4 | BU 1240 | |||||
Aur | 41 Aur | V | 6,2 | 6,9 | 7,5″ | 2019 | STF 845 | 06116+4843 | 100 | |||||||
Aur | 54 Aur | V | 6,2 | 7,9 | 0,8″ | 2016 | STT 152 | 06396+2816 | 260 | |||||||
Aur | 60 Aur | V | 6,5 | 9,0 | 0,2″ | 2012 | 270 a | A8 | G0 | 1,7 | 1,1 | COU 1877 | 06532+3826 | 70 | [11] (S, M) | |
Aur | WW Aur | E/SB | 5,8 | . | – | – | 2,53 d | A5m | A7m | 2,0 | 1,8 | 91 | [30] (V), [33] (U, S, M) | |||
Aur | Gliese 268 | SB | 11,5 | . | – | – | 10,4 d | dM5e | dM5e | 0,2 | 0,2 | 6,3 | [30] (V), [3] (U, S), [48] (M, d) | |||
Boo | δ Boo | CPM | 3,6 | 7,9 | 105,0″ | 2017 | 76 000 a | G8 IIIFe | G0 Vv | STFA 27 | 15155+3319 | 37 | ||||
Boo | ε Boo (Izar) | V | 2,6 | 4,8 | 2,7″ | 2020 | K0 II–III | A2 V | STF 1877 | 14450+2704 | 62 | |||||
Boo | ζ Boo | V | 4,5 | 4,5 | 0,3″ | 2019 | 125 a | A2 III | A2 III | Σ ≈ 2,3 | STF 1865 | 14411+1344 | 54 | [24] (S), [12] (M) | ||
Boo | η Boo | SB/A | 2,7 | . | – | – | 1,4 a | 1,7 | 0,6 | eta Boo | 13547+1824 | 11,4 | [18] (M) | |||
Boo | ι Boo | CPM | 4,8 | 7,4 | 39,0″ | 2020 | A7 V | K1 V | STFA 26 | 14162+5122 | 29 | |||||
Boo | κ Boo | 1 (κ2 = A / κ1 = B) | V | 4,5 | 6,6 | 13,8″ | 2019 | 10 100 a | A7 IV | F2 V | STF 1821 | 14135+5147 | 49 | [3] (UBa/Bb) | ||
2 (Ba/Bb) | SB | 6,6 | . | – | – | 4,9 a | ||||||||||
Boo | μ Boo | 1 (μ1 = A / μ2 = B) | CPM | 4,3 | 7,0 | 109,0″ | 2018 | F0 IV | G0 V | Σ 3,2 ± 0,3 | STFA 28 | 15245+3723 | 36 | [9] (M) | ||
2 (Aa/Ab) | SI | 4,3 | . | 0,1″ | 2012 | 3,7 a | F0 IV | 3,2 ± 0,3 | CHR 181 | |||||||
2 (Ba/Bb) | V | 7,1 | 7,6 | 2,3″ | 2019 | 270 a | G0 V | STF 1938 | ||||||||
Boo | ν2 Boo | SI | 5,8 | 5,8 | 0,1″ | 2015 | 9,0 a | B9 | A1 | 3,0 | 2,3 | A 1634 | 15318+4054 | 130 | [11] (S, M) | |
Boo | ξ Boo | V | 4,8 | 7,0 | 5,2″ | 2020 | 153 a | G8 V | K4 V | 0,9 | 0,7 | STF 1888 | 14514+1906 | 6,7 | [49] (S, M) | |
Boo | π1 Boo | V | 4,9 | 5,8 | 5,4″ | 2020 | STF 1864 | 14407+1625 | 88 | |||||||
Boo | τ Boo | V | 4,5 | 11,1 | 1,5″ | 2017 | 960 a | F7 IV–V | M3 V | 1,4 | 0,4 | STT 270 | 13473+1727 | 16 | [50] (M) | |
Boo | 44 Boo | 1 (A/BC) | V | 5,2 | 6,1 | 0,3″ | 2019 | 210 a | G1 V | G | 1,0 | Σ 1,6 | STF 1909 | 15038+4739 | 13 | [51] (UB/C, S, M) |
2 (B/C) | E/SB | 6,1 | . | – | – | 0,27 d | G | 1,0 | 0,6 | |||||||
Boo | 1 Boo | V | 5,8 | 9,6 | 4,4″ | 2019 | A1 V | A2 | STF 1772 | 13407+1957 | 98 | |||||
Boo | 3 Boo | SB | 6,0 | . | – | – | 36,0 d | G0 IV | F2p | 1,8 | 1,6 | 95 | [30] (V), [5] (S, M) | |||
Boo | 12 Boo | I/SB | 4,8 | . | – | – | 9,60 d | F8 IV | F9 IVw | 1,4 | 1,4 | ISO 14 | 14104+2506 | 36 | [33] (S, M) | |
Boo | 15 Boo | V | 5,4 | 8,4 | 0,8″ | 2015 | KUI 66 | 14148+1006 | 84 | |||||||
Boo | 39 Boo | V | 6,3 | 6,7 | 2,6″ | 2020 | 2100 a | F6 V | F5 V | STF 1890 | 14497+4843 | 69 | [13] (S) | |||
Boo | HP Boo | 1 (A/BC) | V(aO) | 5,9 | 13,9 | 2,6″ | 2009 | 28 000 a | G2 V | L4 + L4 | 1,0 | Σ 0,11 | POT 1 | 14503+2355 | 18 | [52] (S, M) |
2 (B/C) | V(aO) | 13,9 | 14,2 | 0,1″ | 2013 | 10,3 a | L4 | L4 | 0,06 | 0,05 | POT 1 | |||||
Boo | HR 5138 | V | 6,4 | 6,5 | 0,1″ | 2020 | 22,5 a | F0 IV | F2 IV | Σ 2,4 ± 0,4 | BU 612 | 13396+1045 | 60 | [24] (S), [53] (M) | ||
Boo | HR 5386 | 1 (A/BC) | V | 5,0 | 6,8 | 6,4″ | 2020 | A0 V | F0 V + F2 V | STF 1835 | 14234+0827 | 69 | [24] (SB/C) | |||
2 (B/C) | V | 7,4 | 7,7 | 0,3″ | 2020 | 40 a | F0 V | F2 V | BU 1111 | |||||||
Cae | γ1 Cae | V | 4,7 | 8,2 | 3,2″ | 2001 | JC 9 | 05044-3529 | 56 | |||||||
Cam | 1 Cam | O? | 5,8 | 6,8 | 10,4″ | 2018 | O9,7 IIn | B1 IV: | STF 550 | 04320+5355 | 770 | |||||
Cam | 2 Cam | 1 (AB/C) | V | 5,6 | 7,5 | 0,8″ | 2016 | 480 a | STF 566 | 04400+5328 | 65 | |||||
2 (A/B) | V | 5,9 | 7,4 | 0,0″ | 2014 | 26,7 a | STF 566 | |||||||||
Cam | 7 Cam | 1 (A/B) | V | 4,5 | 7,9 | 0,6″ | 2011 | 2700 a | D 5 | 04573+5345 | 110 | [3] (UAa/Ab) | ||||
2 (Aa/Ab) | SB | 4,5 | . | – | – | 3,89 d | ||||||||||
Cam | 11 / 12 Cam | 1 (11 / 12 Cam) | CPM | 5,2 | 6,2 | 177,7″ | 2017 | B3 Ve | K0 IIIe | Σ 1,6 | STFA 13 | 05061+5858 | 220 | [54] (U, M) | ||
2 (12 Cam) | SB | 6,2 | . | – | – | 80,9 d | K0 IIIe | 1,1 | 0,5 | |||||||
Cam | 19 Cam | V | 6,2 | 9,8 | 1,5″ | 2015 | HU 1107 | 05373+6409 | 98 | |||||||
Cam | HR 4892 | 1 (A/B) | V | 5,3 | 5,7 | 21,8″ | 2017 | A0 V | A2 V | STF 1694 | 12492+8325 | 130 | [3] (UAa/Ab) | |||
2 (Ba/Bb) | SB | 5,7 | . | – | – | 3,29 d | A2 V | |||||||||
Cam | Stein 2051 | V | 11,4 | 12,1 | 11,0″ | 2020 | 1800 a | M4 Ve | DC5 | 0,2 | 0,7 | STI 2051 | 04312+5858 | 5,5 | [55] (M) | |
Cap | α Cap (Algiedi) | - (α2 / α1) | O | 3,7 | 4,3 | 381,2″ | 2012 | G9 III | G3 Ib | STFA 51 | 20181-1233 | 32 | ||||
1 (α1 Cap Aa/Ab) | V | 4,4 | 8,6 | 0,8″ | 2002 | G3 Ib | WZ 15 | 20176-1230 | 270 | |||||||
Cap | β Cap (Dabih) | 1 (β1 = A / β2 = B) | CPM | 3,2 | 6,1 | 205,4″ | 2012 | K0 II–III + B8 V + G: V: | B9–A0 III–IV | Σ 7,9 ± 0,4 | STFA 52 | 20210-1447 | 170 | [3] (UAb1/Ab2), [56] (SAa/Ab, SAb1/Ab2, M) | ||
2 (Aa/Ab) | SI/SB | 3,1 | 4,9 | 0,0″ | 2019 | 3,8 a | K0 II–III | B8 V | 3,7 ± 0,2 | Σ 4,2 ± 0,2 | BLA 7 | |||||
2 (Ba/Bb) | V | 6,2 | 9,1 | 0,4″ | 2020 | 540 a | B9–A0 III–IV | BAR 12 | ||||||||
3 (Ab1/Ab2) | SB | 4,9 | . | – | – | 8,68 d | B8 V | G: V: | ≤ 3,4 | ≥ 0,8 | ||||||
Cap | γ Cap | A | 3,7 | . | – | – | 2,2 a | gam Cap | 21401-1640 | 48 | ||||||
Cap | ζ Cap | SB/A | 3,8 | . | – | – | 6,5 a | G8 IIIp | DA2,2 | zet Cap | 21267-2225 | 120 | [46] (S) | |||
Cap | η Cap | SI | 5,0 | 7,4 | 0,3″ | 2020 | 27,9 a | A4 V | F2 V | 2,0 ± 0,2 | 1,2 ± 0,1 | FIN 328 | 21044-1951 | 51 | [12] (S), [16] (M, d) | |
Cap | ο Cap | V | 5,9 | 6,7 | 22,0″ | 2019 | A1 V | A7–8 V | SHJ 324 | 20299-1835 | 72 | |||||
Cap | π Cap | V | 5,1 | 8,5 | 3,5″ | 2019 | BU 60 | 20273-1813 | 200 | |||||||
Cap | ρ Cap | V | 5,0 | 6,9 | 1,7″ | 2018 | 380 a | SHJ 323 | 20289-1749 | 30 | ||||||
Cap | τ Cap | V | 5,4 | 7,3 | 0,4″ | 2019 | 420 a | B4 IV | B6 IV | HU 200 | 20393-1457 | 350 | [24] (S) | |||
Car | ε Car (Avior) | SI | 2,3 | 3,9 | 0,4″ | 2019 | K3: III | B2: V | HDS 1190 | 08225-5931 | 190 | |||||
Car | θ Car | SB/A | 2,8 | . | – | – | 2,2 a | B0,2 V | ≈ 15 | the Car | 10430-6424 | 140 | [57] (S, M) | |||
Car | υ Car | V | 3,0 | 6,0 | 5,1″ | 2015 | RMK 11 | 09471-6504 | 440 | |||||||
Car | 128 G. Car | 1 (AB/C) | V | 5,4 | 12,3 | 18,8″ | 2015 | F3–4 V + F8–G7 V | Σ 2,5 ± 0,6 | I 358 | 09173-6841 | 34 | [16] (S, M, d) | |||
2 (A/B) | SI | 5,8 | 7,1 | 0,1″ | 2020 | 3,4 a | F3–4 V | F8–G7 V | 1,4 ± 0,3 | 1,1 ± 0,3 | FIN 363 | |||||
Car | b1 Car | CPM | 4,9 | 6,6 | 40,1″ | 2010 | B2 V | B8 IV: | DUN 74 | 08570-5914 | 240 | |||||
Car | e2 Car | SI | 5,1 | 8,0 | 0,3″ | 2015 | HDS 1233 | 08353-5801 | 69 | |||||||
Car | V415 Car | E/SB/A | 4,5 | 7,7 | – | – | 195 d | G6 II | A1 V | 3,2 | 2,0 | V415 Car | 06499-5337 | 170 | [5] (S, M) | |
Car | HR 2814 | V | 6,0 | 6,5 | 9,1″ | 2015 | 1 000 000 a | F5 V | F9 V | RMK 6 | 07204-5219 | 37 | ||||
Car | HR 3863 | V | 5,9 | 6,5 | 0,1″ | 2019 | 10,6 a | A3 IV | Σ 5,8 ± 0,6 | B 780 | 09407-5759 | 68 | [58] (M) | |||
Cas | γ Cas | 1 (A/B) | V | 2,2 | 10,9 | 2,1″ | 2002 | B0,5 IVe | F6 V | Σ ≈ 16 | BU 1028 | 00567+6043 | 190 | [59] (UAa/Ab, SA, M), [60] (SB) | ||
2 (Aa/Ab) | SB | 2,2 | . | – | – | 204 d | B0,5 IVe | ≈ 15 | ≈ 0,8 | |||||||
Cas | η Cas | V | 3,5 | 7,4 | 13,6″ | 2020 | 480 a | G3 V | K7 V | 1,0 | 0,6 | STF 60 | 00491+5749 | 6,0 | [49] (S, M) | |
Cas | ι Cas | 1 (AB/C) | V | 4,5 | 9,1 | 6,7″ | 2015 | A3 + G6 + F5 | K4 + M2 | STF 262 | 02291+6724 | 41 | [61][62] (S, M) | |||
2 (A/B) | V | 4,6 | 6,9 | 2,9″ | 2017 | 2400 a | A3 + G6 | F5 | Σ 2,7 ± 0,4 | STF 262 | ||||||
2 (Ca/Cb) | V(aO) | 9,1 | . | 0,2″ | 2018 | K4 | M2 | CTU 2 | ||||||||
3 (Aa/Ab) | SI | 4,6 | 8,5 | 0,6″ | 2010 | 48 a | A3 | G6 | 2,0 ± 0,3 | 0,7 | CHR 6 | |||||
Cas | λ Cas | V | 5,3 | 5,6 | 0,2″ | 2010 | 250 a | B7,5 V | B8,5 V | 3,4 | 3,1 | STT 12 | 00318+5431 | 120 | [24] (S), [11] (M) | |
Cas | μ Cas | SI/SB | 5,3 | 10,7 | 0,6″ | 2016 | 21,6 a | G5 V | dM | 0,7 | 0,2 | WCK 1 | 01083+5455 | 7,6 | [63] (S, M) | |
Cas | ο Cas | I/SB | 4,6 | 7,5 | – | – | 2,8 a | NOI 3 | 00447+4817 | 220 | ||||||
Cas | σ Cas | V | 5,0 | 7,2 | 3,1″ | 2017 | STF 3049 | 23590+5545 | 1400 | |||||||
Cas | 6 Cas | V | 5,7 | 8,0 | 1,5″ | 2015 | STT 508 | 23488+6213 | 1900 | |||||||
Cas | 47 Cas | SI | 5,4 | 7,6 | 0,1″ | 2014 | 4,4 a | LSC 19 | 02051+7717 | 33 | ||||||
Cas | 48 Cas | 1 (AB/C) | CPM | 4,5 | 13,2 | 22,8″ | 2015 | A2 V + F2 V | Σ 3,1 | BU 513 | 02020+7054 | 35 | [24] (S), [64] (M) | |||
2 (A/B) | V/SB | 4,7 | 6,7 | 0,6″ | 2013 | 61 a | A2 V | F2 V | 1,9 | 1,2 | BU 513 | |||||
Cas | 55 Cas | SI | 6,4 | 7,6 | 0,1″ | 2011 | 41 a | F9 II | A2 Vn | MCA 6 | 02145+6631 | 290 | ||||
Cas | AR Cas | 1 (AB/CD) | CPM | 4,9 | 7,2 | 75,0″ | 2018 | B3 V | B9 V | SHJ 355 | 23300+5833 | 180 | [65] (UAa/Ab, SAa/Ab, MAa/Ab) | |||
2? (AB/F) | CPM | 4,9 | 10,6 | 67,2″ | 2012 | B3 V | A0 | HJ 1888 | ||||||||
2? (AB/G) | CPM | 4,9 | 11,1 | 66,9″ | 2012 | B3 V | B3 | HJ 1888 | ||||||||
2 (A/B) | V | 4,9 | 9,3 | 0,9″ | 2002 | B3 V | Σ 7,8 | STT 496 | ||||||||
2 (C/D) | V | 7,2 | 9,1 | 1,3″ | 2015 | B9 V | DA 2 | |||||||||
3 (Aa/Ab) | E/SB | 4,9 | . | – | – | 6,07 d | B4 V | A6 V | 5,9 | 1,9 | ||||||
Cas | V773 Cas | 1 (A/B) | V | 6,3 | 8,7 | 0,6″ | 2010 | 185 a | A3 V | F0–5 | BU 870 | 01443+5732 | 87 | [21] (UAa/Ab) | ||
2 (Aa/Ab) | E | 6,3 | . | – | – | 1,29 d | A3 V | |||||||||
Cas | HR 5 | 1 (A/B) | V | 6,4 | 7,3 | 1,5″ | 2020 | 107 a | G4 V | K0 V + M2 V | 0,9 | Σ 1,3 | STF 3062 | 00063+5826 | 21 | [3] (UBa/Bb), [2] (S, M) |
2 (Ba/Bb) | SB | 7,3 | . | – | – | 47,7 d | K0 V | M2 V | 0,8 | 0,5 | ||||||
Cen | α Cen (Alpha Centauri) | 1 (AB / C = Proxima Centauri) | CPM | −0,3 | 11,1 | 2,2° | – | 550 000 a | G2 V + K1 V | M5,5 V | Σ 2,0 | 0,12 | LDS 494 | 14396-6050 | 1,3 | [33] (SA/B, MA/B), [66] (SC, MC) |
2 (A/B) | V/SB | 0,0 | 1,3 | 5,2″ | 2019 | 80 a | G2 V | K1 V | 1,1 | 0,9 | RHD 1 | |||||
Cen | β Cen (Agena) | 1 (A/B) | V | 0,6 | 4,0 | 0,3″ | 2018 | ≈ 170 a | B1 III + B1 III | B | Σ 22,6 ± 0,3 | VOU 31 | 14038-6022 | 120 | [67] (UA/B, S, M) | |
2 (Aa/Ab) | I/SB | 1,3 | 1,4 | – | – | 357 d | B1 III | B1 III | 12,0 | 10,6 | RBT 1 | |||||
Cen | γ Cen | V | 2,8 | 2,9 | 0,4″ | 2020 | 84 a | A0 III | A0 III | HJ 4539 | 12415-4858 | 40 | [24] (S) | |||
Cen | δ Cen | O | 2,5 | 4,4 | 269,1″ | 1999 | B2 Vne | B3–5 III | JC 2 | 12084-5043 | 130 | |||||
Cen | κ Cen | 1 (A/B) | V | 3,1 | 11,5 | 4,0″ | 2000 | I 1260 | 14592-4206 | 120 | ||||||
2 (Aa/Ab) | SI | 3,3 | 4,7 | 0,1″ | 2020 | 59 a | HDS 2116 | |||||||||
Cen | π Cen | V | 4,1 | 5,7 | 0,3″ | 2019 | 39 a | B9 V | 6,4 | 3,7 | I 879 | 11210-5429 | 110 | [68] (S, M) | ||
Cen | d Cen | V | 4,6 | 5,0 | 0,2″ | 2020 | 83 a | G7 III | G9 III | SEE 179 | 13310-3924 | 280 | [24] (S) | |||
Cen | D Cen | V | 5,8 | 7,0 | 2,7″ | 2015 | RMK 14 | 12140-4543 | 180 | |||||||
Cen | Q Cen | V | 5,2 | 6,5 | 5,6″ | 2016 | B8,5 Vn | A2,5 Va | DUN 141 | 13417-5434 | 83 | |||||
Cen | y Cen | V | 6,3 | 6,4 | 1,0″ | 2020 | 360 a | F0 | F1 | 1,5 | 1,5 | HWE 28 | 13535-3540 | 52 | [11] (S, M) | |
Cen | 3 Cen | O | 4,5 | 6,0 | 7,8″ | 2015 | B5 III | B9 IV | H 3 101 | 13518-3300 | 110 | |||||
Cen | 4 Cen | 1 (A/B) | V | 4,7 | 8,5 | 14,8″ | 2013 | B5 IVp | A3 Vm | H N 51 | 13532-3156 | 170 | [3] (U) | |||
2 (Aa/Ab) | SB | 4,7 | . | – | – | 6,93 d | B5 IVp | |||||||||
2 (Ba/Bb) | SB | 8,5 | . | – | – | 4,84 d | A3 Vm | |||||||||
Cen | 46 Cen | V | 5,2 | 7,7 | 1,3″ | 1995 | HJ 4409 | 11073-4238 | 89 | |||||||
Cen | V831 Cen | 1 (AB/C) | V | 4,6 | 8,4 | 1,9″ | 2019 | ≈ 2000 a | B8 V | Σ 9,4 | ≈ 1,5 | I 424 | 13123-5955 | 110 | [69] (UAB/C, UAa/Ab, S, M, d) | |
2 (A/B) | V | 5,3 | 6,0 | 0,1″ | 2019 | 27,4 a | B8 V | Σ 7,4 | ≈ 2,0 | SEE 170 | ||||||
3 (Aa/Ab) | E/SB | 5,3 | . | – | – | 0,64 d | B8 V | 4,1 | 3,3 | |||||||
Cen | HR 4453 | V | 6,1 | 6,2 | 0,5″ | 2019 | I 78 | 11336-4035 | 120 | |||||||
Cep | β Cep | 1 (A/B) | V | 3,2 | 8,6 | 13,5″ | 2016 | B2 III + B5 Ve | A0 V | Σ 17 ± 4 | 3,1 ± 0,3 | STF 2806 | 21287+7034 | 210 | [70] (SAa/Ab, MAa/Ab), [2] (SB, MB) | |
2 (Aa/Ab) | SI/SB | 3,2 | 6,6 | 0,2″ | 2007 | 83 a | B2 III | B5 Ve | 12,6 ± 3,2 | 4,4 ± 0,7 | LAB 6 | |||||
Cep | γ Cep | V(aO)/SB | 3,2 | > 7,3 | 0,9″ | 2006 | 68 a | K1 III–IV | M4 | 1,4 | 0,4 | NHR 9 | 23393+7738 | 14 | [13] (V1), [71] (S, M) | |
Cep | κ Cep | V | 4,4 | 8,3 | 7,3″ | 2015 | B9 III | A7 V | STF 2675 | 20089+7743 | 99 | |||||
Cep | ξ Cep | 1 (A/B) | V | 4,5 | 6,4 | 8,1″ | 2019 | 2500 a | kA2,5hF2mF2(IV) | F8 V | Σ 1,4 | STF 2863 | 22038+6438 | 30 | [10] (M) | |
2 (Aa/Ab) | SI/SB | 4,8 | 6,3 | 0,1″ | 2012 | 2,2 a | kA2,5hF2mF2(IV) | 1,0 | 0,4 | MCA 69 | ||||||
Cep | ο Cep | V | 5,0 | 7,3 | 3,4″ | 2018 | 2200 a | STF 3001 | 23186+6807 | 62 | ||||||
Cep | π Cep | 1 (A/B) | V | 4,6 | 6,8 | 1,1″ | 2016 | 176 a | G2 III | A9 V | Σ 6,9 ± 0,7 | 1,9 ± 0,2 | STT 489 | 23079+7523 | 76 | [72] (S, M) |
2 (Aa/Ab) | SB/A | 4,4 | . | – | – | 1,5 a | G2 III | 3,6 ± 0,5 | 3,3 ± 0,5 | |||||||
Cep | VV Cep | E/SB | 5,4 | . | – | – | 20,3 a | M2 Iab | B | 2,5 vs. 20 | 8 vs. 20 | WRH 36 | 21567+6338 | 1500 | [73][74] (M), [75] (S, d) | |
Cep | HR 1230 | V | 5,6 | 6,3 | 0,8″ | 2012 | 370 a | G8 III | A3,5 IV: | STF 460 | 04100+8042 | 120 | ||||
Cep | HR 8357 | O | 5,6 | 6,4 | 18,1″ | 2018 | STF 2840 | 21520+5548 | 200 | |||||||
Cep | Kruger 60 | V | 9,9 | 11,4 | 1,5″ | 2016 | 44,7 a | M3 V | M4 V | 0,3 | 0,18 | KR 60 | 22280+5742 | 4,0 | [76] (M) | |
Cet | γ Cet | 1 (AB/C) | CPM | 3,5 | 10,2 | 843,1″ | 2000 | A2 Vn + F4 V | K5 V | ALD 124 | 02433+0314 | 24 | ||||
2 (A/B) | V | 3,5 | 6,2 | 1,9″ | 2020 | A2 Vn | F4 V | STF 299 | ||||||||
Cet | ε Cet | SI/SB | 5,2 | 6,5 | 0,1″ | 2020 | 2,7 a | F2 V | F7–G4 V | 1,4 | 1,0 | FIN 312 | 02396-1152 | 24 | [16] (S, M) | |
Cet | μ Ceti | SI/SB | 4,2 | 6,2 | 0,2″ | 2020 | 3,3 a | A9 IIIP | TOK 1 | 02449+1007 | 26 | [3] (U) | ||||
Cet | ν Cet | 1 (A/B) | V | 5,0 | 9,1 | 8,4″ | 2011 | STF 281 | 02359+0536 | 100 | [3] (UAa/Ab) | |||||
2 (Aa/Ab) | SB | 5,0 | . | – | – | 2,0 a | ||||||||||
Cet | ξ1 Cet | SI/SB | 4,3 | . | 0,1″ | 2007 | 4,5 a | MCA 5 | 02130+0851 | 100 | ||||||
Cet | ο Cet (Mira) | V | 6,8 | 10,4 | 0,5″ | 2014 | 500 a | M5–9 IIIe | DA | 1,2 | JOY 1 | 02193-0259 | 92 | [77] (M) | ||
Cet | 10 Cet | SI | 6,5 | 8,9 | 0,5″ | 2020 | HDS 61 | 00266-0003 | 140 | |||||||
Cet | 13 Cet | 1 (A/B) | V/SB | 5,6 | 6,9 | 0,2″ | 2020 | 6,9 a | F9 V + K0 V | G6 V | Σ 1,8 | 0,9 | HO 212 | 00352-0336 | 21 | [3] (UAa/Ab), [2] (S, M) |
2 (Aa/Ab) | SB | 5,6 | . | – | – | 2,08 d | F9 V | K0 V | 1,0 | 0,8 | ||||||
Cet | 26 Cet | V | 6,1 | 9,5 | 16,0″ | 2015 | A8 IV | G8 V | STF 84 | 01038+0122 | 59 | |||||
Cet | 37 Cet | 1 (A/B) | CPM | 5,2 | 7,9 | 47,1″ | 2018 | STFA 3 | 01144-0755 | 24 | ||||||
2 (Aa/Ab) | SI | 5,2 | 9,7 | 0,2″ | 2013 | WSI 70 | ||||||||||
Cet | 42 Cet | 1 (A/BC) | V | 6,5 | 7,0 | 1,6″ | 2020 | 650 a | G8 III | A7 V + A: | Σ 1,8 ± 0,6 | STF 113 | 01198-0031 | 100 | [20] (S, M) | |
2 (B/C) | SI | 7,4 | 7,6 | 0,1″ | 2020 | 27 a | A7 V | A: | 1,8 ± 0,6 | FIN 337 | ||||||
Cet | 84 Cet | V | 5,8 | 9,7 | 3,6″ | 2012 | 3200 a | STF 295 | 02412-0042 | 23 | ||||||
Cet | 94 Cet | V | 5,1 | 11,0 | 2,2″ | 2015 | 1400 a | HJ 663 | 03128-0112 | 23 | ||||||
Cet | 95 Cet | V | 5,6 | 8,0 | 1,2″ | 2017 | 390 a | K0 IV | G8 V | AC 2 | 03184-0056 | 64 | [24] | |||
Cet | HR 159 | V/SB | 6,6 | 6,2 | 0,2″ | 2020 | 25,0 a | G8 V | G8 V | 0,9 | 0,7 | BU 395 | 00373-2446 | 15 | [1] (S, M, d) | |
Cet | HR 492 | V | 6,1 | 7,2 | 0,1″ | 2020 | 630 a | F5 V | F7 V | STF 147 | 01417-1119 | 39 | ||||
Cet | GJ 1005 | SI | 11,0 | 11,4 | 0,4″ | 2020 | 4,6 a | M3,5 V | M | 0,18 | 0,12 | HEI 299 | 00155-1608 | 5,0 | [78] (S, M) | |
Cet | Luyten 726-8 | V | 12,7 | 13,2 | 1,9″ | 2020 | 26,3 a | M5,5 V | M6 V | 0,10 | 0,10 | LDS 838 | 01388-1758 | 2,7 | [76] (M) | |
Cha | δ1 Cha | V | 6,2 | 6,5 | 0,8″ | 2019 | I 294 | 10453-8028 | 110 | |||||||
Cha | ε Cha | 1 (AB/C) | CPM | 4,9 | 6,6 | 134,0″ | 2015 | B9 V + B9 V + B9 V | A0 | FGL 1 | 11596-7813 | 110 | [79] (U, S, M) | |||
2 (A/B) | V | 5,3 | 6,0 | 0,2″ | 2020 | ≈ 920 a | B9 V + B9 V | B9 V | Σ ≈ 5 | HJ 4486 | ||||||
3 (Aa/Ab) | SI | 6,0 | 6,2 | 0,0″ | 2020 | 13 a | B9 V | B9 V | ≈ 2,5 | ≈ 2,5 | HJ 4486 | |||||
Cir | α Cir | V | 3,2 | 8,5 | 15,7″ | 2016 | A7 VpSrCrEu | K5 V | DUN 166 | 14425-6459 | 17 | |||||
Cir | γ Cir | V | 4,9 | 5,7 | 0,8″ | 2019 | 260 a | B3–4 V | F8 V | HJ 4757 | 15234-5919 | 140 | ||||
Cir | θ Cir | SI | 5,9 | 5,9 | 0,1″ | 2020 | 40 a | B3 Ve | Σ 40 ± 18 | FIN 372 | 14567-6247 | 460 | [20] (S, M) | |||
Cir | 26 G. Cir | 1 (A/B) | SI | 6,2 | 8,7 | 0,3″ | 2018 | F8 II + B6 | Σ 10,2 | HDS 2100 | 14526-6349 | 530 | [19] (U, S, M, d) | |||
2 (Aa/Ab) | I | 6,2 | . | – | – | 17,9 a | F8 II | B6 | 5,2 | 5,0 | GAA 1 | |||||
CMa | α CMa (Sirius) | V | −1,5 | 8,4 | 11,2″ | 2020 | 50 a | A1 V | DA2 | 2,1 | 1,0 | AGC 1 | 06451-1643 | 2,6 | [80] (S, M) | |
CMa | ε CMa | V | 1,5 | 7,5 | 7,9″ | 2008 | CPO 7 | 06586-2858 | 120 | |||||||
CMa | ζ CMa | - (A/B) | O | 3,0 | 7,8 | 169,6″ | 2016 | B2,5 V | K1 III | SMY 1 | 06203-3004 | 110 | [3] (UAa/Ab) | |||
1 (Aa/Ab) | SI/SB | 3,6 | 3,8 | 0,0″ | 2020 | 1,9 a | B5,5 V | TOK 821 | 06203-3004 | 220 | ||||||
CMa | η CMa | O | 2,5 | 6,8 | 177,0″ | 2020 | B5 Ia | A0 V | SMY 2 | 07241-2918 | 610 | |||||
CMa | μ CMa | V | 5,3 | 7,1 | 2,9″ | 2017 | STF 997 | 06561-1403 | 280 | |||||||
CMa | ν1 CMa | V | 5,8 | 7,4 | 17,4″ | 2019 | G8–K0 III | F–G | SHJ 73 | 06364-1840 | 81 | |||||
CMa | π CMa | V | 4,7 | 9,6 | 11,6″ | 2015 | H N 123 | 06556-2008 | 30 | |||||||
CMa | τ CMa | 1 (A/E) | SI | 4,4 | 9,7 | 0,9″ | 2018 | O9,2 + O9 III | B2: V | TOK 42 | 07187-2457 | 1500 | [81] (U, S, d) | |||
2 (Aa/Ab) | SI | 4,9 | 5,3 | 0,1″ | 2018 | O9,2 | O9 III | FIN 313 | ||||||||
3 (Aa) | SB | 4,9 | . | – | – | 155 d | O9,2 | |||||||||
4 (Aa) | E | 4,9 | . | – | – | 1,28 d | O9,2 | |||||||||
CMa | 27 CMa | SI | 5,4 | 4,9 | 0,1″ | 2020 | 119 a | B4Ve(shell) | FIN 323 | 07143-2621 | 530 | |||||
CMa | 29 CMa (UW CMa) | E/SB | 5,0 | . | – | – | 4,39 d | O7,5–8 Iabf | O9,7 Iab | ≈ 16 | ≈ 19 | 1500 | [82] (U, S, M) | |||
CMa | HR 2522 | V | 5,6 | 7,2 | 0,4″ | 2015 | 580 a | AC 4 | 06490-1509 | 160 | ||||||
CMi | α CMi (Prokyon) | V | 0,5 | 10,8 | 3,8″ | 2014 | 41 a | F5 IV–V | DQZ | 1,5 | 0,6 | SHB 1 | 07393+0514 | 3,5 | [83] (S, M) | |
CMi | η CMi | V | 5,3 | 11,1 | 4,3″ | 2015 | BU 21 | 07280+0657 | 97 | |||||||
CMi | HR 2950 | V | 6,6 | 7,0 | 0,9″ | 2019 | 1250 a | STF 1126 | 07401+0514 | 79 | ||||||
Cnc | ζ Cnc | 1 (ζ1 = AB / ζ2 = CD) | V | 4,9 | 5,9 | 6,0″ | 2020 | 740 a | F8 V + G5 V | G0 V + M2 V | Σ 2,6 | Σ 2,0 | STF 1196 | 08122+1739 | 25 | [18][84] (S, M) |
2 (A/B) | V | 5,3 | 6,3 | 1,2″ | 2020 | 59,4 a | F8 V | G5 V | 1,3 | 1,2 | STF 1196 | |||||
2 (C/D) | SI | 6,2 | 7,1 | 0,3″ | 2020 | 17,3 a | G0 V | M2 V | 1,2 | 0,8 | HUT 1 | |||||
Cnc | ι Cnc | V | 4,1 | 6,0 | 30,7″ | 2018 | G8 IIIa | A2 V | STF 1268 | 08467+2846 | 100 | |||||
Cnc | κ Cnc | SI | 5,3 | 8,8 | 0,1″ | 2019 | CHR 257 | 09077+1040 | 150 | |||||||
Cnc | π1 Cnc | 1 (A/E) | CPM | 6,6 | 17,0 | 43,0″ | 1997 | G8 V + G8 V | L8 + T | Σ 1,8 | Σ ≈ 0,08–0,14 | WIL 1 | 09123+1500 | 20 | [1] (SAa/Ab, MAa/Ab, d), [85] (UEa/Eb, SEa/Eb, MEa/Eb) | |
2 (Aa/Ab) | SI/SB | 7,2 | 7,2 | 0,1″ | 2019 | 2,7 a | G8 V | G8 V | 0,9 | 0,9 | FIN 347 | |||||
2 (Ea/Eb) | V(aO) | 17,0 | . | 0,5″ | 2004 | ≈ 140–180 a | L8 | T | ≈ 0,04–0,07 | ≈ 0,04–0,07 | BUG 16 | |||||
Cnc | φ2 Cnc | V | 6,2 | 6,2 | 5,2″ | 2019 | A5 IV | A2 Vp | STF 1223 | 08268+2656 | 85 | |||||
Cnc | 21 Cnc | V | 6,3 | 9,4 | 1,3″ | 2019 | A 2961 | 08239+1038 | 250 | |||||||
Cnc | 24 Cnc | 1 (A/BC) | V | 6,9 | 7,5 | 5,7″ | 2019 | F0 V | F7 V | STF 1224 | 08267+2432 | 80 | ||||
2 (B/C) | V | 8,5 | 8,5 | 0,2″ | 2007 | 21,8 a | F7 V | A 1746 | ||||||||
Cnc | 55 (ρ1) Cnc | CPM | 6,0 | 13,2 | 85,1″ | 2012 | K0 IV–V | M4,5 V | 1,0 | 0,3 | LDS 6219 | 08526+2820 | 13 | [86] (M1), [87] (M2) | ||
Cnc | 57 Cnc | V | 6,1 | 6,4 | 1,5″ | 2019 | 2300 a | STF 1291 | 08542+3035 | 140 | ||||||
Cnc | 66 Cnc | V | 6,0 | 8,6 | 4,4″ | 2017 | STF 1298 | 09014+3215 | 150 | |||||||
Cnc | 75 Cnc | SB/A | 6,0 | . | – | – | 19,4 d | G5 IV–V | 1,2 | 1,0 | 75 Cnc | 09088+2638 | 31 | [88] (S, M, d) | ||
Cnc | GJ 1116 | V | 13,4 | 13,4 | 2,6″ | 2020 | 124 a | M7 V | M7 V | LDS 3836 | 08582+1945 | 5,3 | ||||
Cnc | HM Cnc | SB | 20 | . | – | – | 0,004 d | D | D | 0,6 | 0,3 | 5000 | [30] (V), [89] (U, S, M, d) | |||
Col | δ Col | SB/A | 3,9 | . | – | – | 2,4 a | del Col | 06221-3326 | 62 | ||||||
Col | HR 2424 | 1 (AB/C) | V | 5,5 | 11,5 | 21,0″ | 1999 | HJ 3875 | 06354-3647 | 160 | ||||||
2 (A/B) | V | 5,9 | 6,9 | 1,6″ | 2015 | BU 755 | ||||||||||
Col | HR 2431 | 1 (A/B) | CPM | 6,4 | 7,3 | 287,2″ | 2015 | F9 V + G1 V | G2 V | Σ 2,3 | Σ 1,9 | SHY 185 | 06359-3605 | 40 | [24] (SAa/Ab), [11] (MAa/Ab), [68] (MBa/Bb) | |
2 (Aa/Ab) | SI | 6,7 | 8,2 | 0,1″ | 2020 | 28,9 a | F9 V | G1 V | 1,2 | 1,1 | FIN 19 | |||||
2 (Ba/Bb) | V | 7,8 | 8,6 | 0,1″ | 2020 | 14,0 a | G1 V | 1,1 | 0,8 | RST 4816 | ||||||
Com | α Com | V | 4,9 | 5,5 | 0,6″ | 2019 | 25,9 a | F5 V | F6 V | 1,2 | 1,1 | STF 1728 | 13100+1732 | 18 | [90] (S, M) | |
Com | 2 Com | V | 6,2 | 7,5 | 3,4″ | 2020 | STF 1596 | 12043+2128 | 100 | |||||||
Com | 12 Com | SB | 4,9 | . | – | – | 1,1 a | G7 III | A3 IV | 2,6 | 2,1 | 12225+2551 | 85 | [5] (S, M) | ||
Com | 23 Com | SI | 5,0 | 6,9 | 0,4″ | 2020 | 36 a | WRH 12 | 12349+2238 | 95 | ||||||
Com | 24 Com | V | 5,1 | 6,3 | 20,2″ | 2018 | K0 II–III | A9 V | STF 1657 | 12351+1823 | 120 | |||||
Com | 35 Com | 1 (AB/C) | V | 5,2 | 9,8 | 28,5″ | 2016 | K0 III + F3 V | STF 1687 | 12533+2115 | 87 | [24] (S), [3] (UAa/Ab) | ||||
2 (A/B) | V | 5,2 | 7,1 | 1,3″ | 2019 | 490 a | K0 III | F3 V | STF 1687 | |||||||
3 (Aa/Ab) | SB | 5,2 | . | – | – | 8,0 a | K0 III | |||||||||
Com | 39 Com | 1 (A/B) | V | 6,0 | 8,8 | 1,8″ | 2019 | COU 11 | 13064+2109 | 50 | ||||||
2 (Aa/Ab) | SI | 6,1 | . | 0,0″ | 2009 | CHR 150 | ||||||||||
Com | Gliese 505 | V | 6,7 | 9,5 | 7,6″ | 2018 | 610 a | K1 V | M1 V | 0,7 | 0,5 | BU 800 | 13169+1701 | 11,0 | [24] (S), [91] (MA), [87] (MB) | |
CrA | γ CrA | V | 4,5 | 6,4 | 1,5″ | 2020 | 122 a | F8 V | F8 V | 1,2 | 1,2 | HJ 5084 | 19064-3704 | 17 | [60] (S), [11] (M) | |
CrA | κ CrA | CPM | 5,6 | 6,2 | 20,5″ | 2018 | B9 V | B8–A1 | DUN 222 | 18334-3844 | 210 | |||||
CrA | HR 6749 | V | 5,7 | 5,7 | 1,8″ | 2019 | 450 a | A5 V | A5 V | HJ 5014 | 18068-4325 | 45 | [24] (S) | |||
CrB | α CrB (Gemma) | E/SB/A | 2,2 | . | – | – | 17,4 d | A0 V | G5 V | 2,6 | 0,9 | alp CrB | 15347+2643 | 23 | [92] (S, M) | |
CrB | β CrB | SI/SB | 3,7 | 5,2 | 0,3″ | 2019 | 10,5 a | A5 | F2 | 2,1 | 1,4 | JEF 1 | 15278+2906 | 34 | [93] (S, M) | |
CrB | γ CrB | V | 4,0 | 5,6 | 0,5″ | 2015 | 91 a | B9 IV | A3 V | 2,8 | 1,7 | STF 1967 | 15427+2618 | 45 | [24] (S), [11] (M) | |
CrB | ζ2 CrB | V | 5,0 | 5,9 | 6,3″ | 2019 | B7 V | B9 V | STF 1965 | 15394+3638 | 150 | |||||
CrB | η CrB | V/SB | 5,6 | 6,0 | 0,4″ | 2019 | 41,6 a | G1 V | G3 V | 1,2 | 1,1 | STF 1937 | 15232+3017 | 18 | [24] (S), [9] (M) | |
CrB | θ CrB | V | 4,3 | 6,3 | 0,8″ | 2016 | COU 610 | 15329+3122 | 120 | |||||||
CrB | σ CrB | 1 (σ2/1 = AB / E) | CPM | 5,1 | 12,3 | 634,8″ | 2015 | F6 V + G1 V | M2,5 V | Σ 3,2 | Σ 0,5 | STF 2032 | 16147+3352 | 21 | [94] (S, M) | |
2 (σ2 = A / σ1 = B) | V | 5,6 | 6,5 | 7,2″ | 2019 | 670 a | F6 V | G1 V | Σ 2,2 | 1,0 | STF 2032 | |||||
2 (Ea/Eb) | SI | 12,4 | 15,0 | 0,5″ | 2018 | 52 a | M2,5 V | 0,4 | 0,1 | YSC 152 | ||||||
3 (Aa/Ab) | I/SB | 5,6 | . | – | – | 1,14 d | F6 V | 1,1 | 1,1 | |||||||
Crt | ζ Crt | SI | 5,0 | 7,8 | 0,3″ | 2018 | HDS 1658 | 11448-1821 | 100 | |||||||
Crt | ψ Crt | V | 6,2 | 8,3 | 0,2″ | 2018 | 370 a | B9 V | A1 V | BU 220 | 11125-1830 | 150 | [24] (S) | |||
Cru | α Cru (Acrux) | 1 (AB/C) | CPM | 0,7 | 4,8 | 89,0″ | 2020 | B0,5 IV + B1 V | B3–5 V | DUN 252 | 12266-6306 | 99 | [3] (UAa/Ab), [95] (UCa/Cb) | |||
2 (α1 = A / α2 = B) | V | 1,3 | 1,6 | 3,5″ | 2020 | B0,5 IV | B1 V | DUN 252 | ||||||||
3 (Aa/Ab) | SB | 1,3 | . | – | – | 75,8 d | B0,5 IV | |||||||||
3 (Ca/Cb) | SB | 4,8 | . | – | – | 1,23 d | B3–5 V | |||||||||
Cru | γ Cru | O | 1,8 | 6,5 | 133,2″ | 2018 | M3,5 III | A3 V | DUN 124 | 12312-5707 | 27 | |||||
Cru | μ Cru | CPM | 3,9 | 5,0 | 34,5″ | 2020 | B2 IV–V | B5 Vne | DUN 126 | 12546-5711 | 130 | |||||
Crv | δ Crv | V | 3,0 | 8,5 | 24,2″ | 2020 | SHJ 145 | 12299-1631 | 27 | |||||||
Crv | VV Crv | 1 (AB/C) | CPM | 5,1 | 10,3 | 45,9″ | 2016 | F5 V + F4 IVn | STF 1669 | 12413-1301 | 77 | [3] (UAa/Ab), [96] (UA/B, UBa/Bb) | ||||
2 (A / B = VV Crv) | V | 5,9 | 5,9 | 5,3″ | 2020 | ≈ 3500 a | F5 V | F4 IVn | STF 1669 | |||||||
3 (Aa/Ab) | SB | 5,9 | . | – | – | 44,5 d | F5 V | Σ 3,5 | ||||||||
3 (Ba/Bb) | E/SB | 5,9 | . | – | – | 3,14 d | F4 IVn | 2,0 | 1,5 | |||||||
CVn | α CVn (Cor Caroli) | V | 2,9 | 5,5 | 19,3″ | 2020 | A0 VpSiEu | F2 V | STF 1692 | 12560+3819 | 35 | |||||
CVn | 2 CVn | V | 5,9 | 8,7 | 11,6″ | 2017 | M0,5 III | F7 V | STF 1622 | 12161+4040 | 200 | |||||
CVn | 17 / 15 CVn | 1 (17 = A / 15 = BC) | O | 6,0 | 6,3 | 275,6″ | 2012 | A9 III–IV | B7 III | STFA 24 | 13101+3830 | 60 | ||||
2 (B/C) | V | 6,3 | 9,2 | 1,3″ | 2016 | B7 III | BU 608 | 13101+3830 | 1140 | |||||||
CVn | 19 CVn | SI | 5,9 | 9,5 | 0,6″ | 2012 | 220 a | CHR 180 | 13155+4051 | 73 | ||||||
CVn | 25 CVn | V | 5,0 | 7,0 | 1,6″ | 2019 | 240 a | A6 III | F0 V | STF 1768 | 13375+3618 | 61 | [24] (S) | |||
CVn | HR 5110 (BH CVn) | E/SB/A | 5,0 | . | – | – | 2,61 d | F2 IV | K0 IV | 1,5 | 0,8 | BH CVn | 13348+3711 | 46 | [97] (S, M) | |
Cyg | β Cyg (Albireo) | 1 (β1 = A / β2 = B) | O? | 3,2 | 4,7 | 34,6″ | 2020 | K3 II + B9,5 V | B8 Ve | Σ 9,5 +5,9−3,3 | 3,7 ± 0,1 | STFA 43 | 19307+2758 | 100 | [98] (U, M) | |
2 (Aa/Ac) | SI | 3,4 | 5,2 | 0,3″ | 2020 | 122 a | K3 II | B9,5 V | 4,2 +2,9−1,6 | 5,2 +3,1−1,7 | MCA 55 | 19307+2758 | 120 | |||
Cyg | δ Cyg | V | 2,9 | 6,3 | 2,7″ | 2017 | 660 a | B9 III | F1 V | STF 2579 | 19450+4508 | 51 | [24] (S) | |||
Cyg | ζ Cyg | V(HST)/ SB |
3,2 | 13,2 | – | – | 17,8 a | G8 IIIp | DA4,2 | BAS 7 | 21129+3014 | 44 | [3] (U), [46] (S) | |||
Cyg | λ Cyg | 1 (A/B) | V | 4,7 | 6,3 | 0,9″ | 2018 | 800 a | B4 V | B7 V | Σ 10,6 | 7,4 | STT 413 | 20474+3629 | 240 | [24] (S), [99] (M) |
2 (Aa/Ab) | SI | 5,4 | 5,8 | 0,0″ | 1991 | 11,6 a | B4 V | 5,3 | 5,3 | MCA 63 | ||||||
Cyg | μ Cyg | V | 4,8 | 6,2 | 1,6″ | 2019 | 690 a | F4 V | G2 V | STF 2822 | 21441+2845 | 22 | [24] (S) | |||
Cyg | ο1 Cyg | E/SI/SB | 3,9 | . | 0,0″ | 1985 | 10,0 a | K4 Ib | B3–4 | 11,7 | 7,1 | WRH 33 | 20136+4644 | 230 | [100] (S, M) | |
Cyg | ο2 Cyg | E/SB/A | 4,2 | 8,4 | – | – | 3,1 a | K4–5 Ib | B6–7 | 9,7 | 4,8 | 20155+4743 | 470 | [100] (S, M) | ||
Cyg | τ Cyg | 1 (AB/F) | CPM | 3,7 | 12,0 | 89,5″ | 2012 | F0 V + G0 V | M3 | Σ 2,7 | AGC 13 | 21148+3803 | 20 | [40] (S), [18] (M) | ||
2 (A/B) | V | 3,8 | 6,6 | 1,1″ | 2017 | 49,5 a | F0 V | G0 V | 1,7 | 1,0 | AGC 13 | |||||
2 (Fa/Fb) | SI | 12,2 | 13,8 | 0,4″ | 2018 | M3 | JOD 20 | |||||||||
Cyg | φ Cyg | SI/SB | 4,9 | 5,1 | 0,0″ | 1994 | 1,2 a | K0 III | K0 III | 2,2 | 2,1 | MCA 57 | 19394+3009 | 74 | [101] (S, M) | |
Cyg | ψ Cyg | 1 (A/B) | V | 5,0 | 7,5 | 2,9″ | 2017 | A2 IV–V | F4 V | STF 2605 | 19556+5226 | 85 | [24] (S) | |||
2 (Aa/Ab) | SI | 5,6 | 6,1 | 0,1″ | 2010 | 54 a | F4 V | YR 2 | ||||||||
Cyg | 9 Cyg | SI/SB | 5,9 | 6,5 | 0,0″ | 1994 | 4,6 a | G8 IIIa | A2 V | 2,8 | 2,6 | WRH 32 | 19348+2928 | 180 | [5] (S, M) | |
Cyg | 16 Cyg | 1 (AC/B) | V | 6,0 | 6,2 | 39,7″ | 2020 | 13 500 a | G1,5 Vb + M | G2,5 V | Σ 1,5 | 1,0 | STFA 46 | 19418+5032 | 21 | [13] (SA/B), [102] (UA/C, SC, MC), [103] (MA/B) |
2 (A/C) | V(aO) | 6,0 | 13,0 | 3,2″ | 2009 | ≈ 700 a | G1,5 Vb | M | 1,1 | ≈ 0,4 | TRN 4 | |||||
Cyg | 17 Cyg | 1 (AB/FG) | CPM | 5,1 | 7,8 | 817,6″ | 2010 | 3 700 000 a | F5,5 IV–V + K4 | K5 V + K5 V | STF 2580 | 19464+3344 | 21 | |||
2 (A/B) | V | 5,1 | 9,3 | 25,9″ | 2020 | 7900 a | F5,5 IV–V | K4 | STF 2580 | |||||||
2 (F/G) | V | 8,5 | 8,6 | 3,2″ | 2020 | 230 a | K5 V | K5 V | STF 2576 | |||||||
Cyg | 44 Cyg | V | 6,3 | 10,1 | 2,2″ | 1991 | AC 18 | 20310+3656 | 1200 | |||||||
Cyg | 47 Cyg | SI | 4,8 | 7,3 | 0,3″ | 1998 | K6: Ib | B2,5: | WRH 34 | 20339+3515 | 1300 | |||||
Cyg | 49 Cyg | V | 5,8 | 8,1 | 2,7″ | 2016 | G8 IIb | B9,9 | STF 2716 | 20410+3218 | 270 | |||||
Cyg | 52 Cyg | V | 4,3 | 9,5 | 5,9″ | 2018 | STF 2726 | 20456+3043 | 62 | |||||||
Cyg | 59 Cyg | SI | 4,8 | 7,6 | 0,1″ | 2015 | 162 a | MCA 65 | 20598+4731 | 400 | ||||||
Cyg | 60 Cyg | V | 5,4 | 9,5 | 2,9″ | 2017 | STT 426 | 21012+4609 | 490 | |||||||
Cyg | 61 Cyg | V | 5,2 | 6,1 | 31,8″ | 2019 | 620 a | K5 V | K7 V | 0,7 | 0,6 | STF 2758 | 21069+3845 | 3,5 | [104] (S, M) | |
Cyg | 75 Cyg | V | 5,3 | 10,1 | 2,7″ | 2008 | AC 20 | 21402+4316 | 130 | |||||||
Cyg | 77 Cyg | 1 (AB/C) | CPM | 5,8 | 7,8 | 145,5″ | 2017 | A0 V + A0 V | F2 | ARY 129 | 21424+4105 | 130 | ||||
2 (A/B) | V | 6,3 | 6,7 | 0,2″ | 2014 | 26,5 a | A0 V | A0 V | KUI 108 | |||||||
2 (Ca/Cb) | V | 8,1 | 8,6 | 0,5″ | 2016 | F2 | BU 688 | 21424+4103 | ||||||||
Cyg | HR 7294 | V | 6,5 | 6,7 | 7,2″ | 2020 | 1460 a | G3 V | G2 V | STF 2486 | 19121+4951 | 25 | ||||
Cyg | HR 7911 | V | 6,7 | 6,8 | 0,9″ | 2018 | 1150 a | STT 410 | 20396+4035 | 280 | ||||||
Cyg | GJ 1245 | 1 (AC/B) | V | 13,5 | 16,8 | 6,0″ | 2019 | 220 a | M5 + M8,5 | M6 V | Σ 0,19 | GIC 159 | 19539+4425 | 4,7 | [105] (SA/C), [78] (MA/C) | |
2 (A/C) | SI | 14,3 | 15,0 | 0,5″ | 2016 | 16,8 a | M5 | M8,5 | 0,11 | 0,08 | MCY 3 | |||||
Del | α Del | 1 (Aa/Ab) | SI | 3,9 | 6,4 | 0,2″ | 2014 | 16,9 a | B9 IV | 3,8 ± 0,4 | Σ 3,3 ± 0,3 | WCK 2 | 20396+1555 | 78 | [106] (U, M) | |
2 (Ab1/Ab2) | A | 6,4 | . | – | – | 30,0 d | 1,8 ± 0,2 | 1,5 ± 0,1 | ||||||||
Del | β Del | V/SB | 4,1 | 5,0 | 0,2″ | 2018 | 26,7 a | F5 III | F5 IV | 1,8 | 1,5 | BU 151 | 20375+1436 | 31 | [24] (S), [107] (M) | |
Del | γ Del | V | 4,4 | 5,0 | 8,9″ | 2019 | 3200 a | K1 IV | F8 V | STF 2727 | 20467+1607 | 35 | ||||
Del | δ Del | SB/A | 4,4 | . | – | – | 40,6 d | 1,8 | 1,6 | 64 | [30] (V), [108] (U, M) | |||||
Del | 1 Del | V | 6,2 | 8,0 | 0,9″ | 2016 | Be(shell) | B | BU 63 | 20303+1054 | 230 | [109] (S) | ||||
Del | 13 Del | V | 5,6 | 8,2 | 1,5″ | 2009 | BU 65 | 20478+0600 | 140 | |||||||
Dor | α Dor | V | 3,6 | 4,6 | 0,2″ | 2020 | 12,1 a | A0 IIIp | B9 IV | B 2092 | 04340-5503 | 52 | [13] (S) | |||
Dra | α Dra (Thuban) | SB/A | 3,8 | 5,6 | – | – | 51,4 d | A0 III | A2: | 2,8 | ≈ 2,6 | alp Dra | 14044+6423 | 93 | [110] (V), [111] (S, M) | |
Dra | ε Dra | V | 4,0 | 6,9 | 3,2″ | 2017 | 2800 a | G7 IIIb | F5 III | STF 2603 | 19482+7016 | 47 | ||||
Dra | ζ Dra | SI | 3,2 | 4,2 | 0,1″ | 1994 | 6,6 a | 5,9 ± 1,2 | 3,6 ± 0,8 | STA 1 | 17088+6543 | 100 | [112] (M) | |||
Dra | η Dra | V | 2,8 | 8,2 | 4,4″ | 2015 | STT 312 | 16240+6131 | 28 | |||||||
Dra | μ Dra | 1 (AB/C) | V | 4,9 | 13,7 | 12,2″ | 2015 | F7 V + F7 V + G4 V | M3: | Σ 3,2 | STF 2130 | 17053+5428 | 27 | [13] (SA), [2] (SBa/Bb, M) | ||
2 (A/B) | V | 5,7 | 5,7 | 2,7″ | 2020 | 420 a | F7 V | F7 V + G4 V | 1,2 | Σ 1,8 | BU 1088 | |||||
3 (Ba/Bb) | SB | 5,7 | . | – | – | 3,2 a | F7 V | G4 V | 1,1 | 0,9 | ||||||
Dra | ν Dra | CPM | 4,9 | 4,9 | 62,1″ | 2017 | kA3hF0mF0(IV–V) | kA4hF2VmF3 | STFA 35 | 17322+5511 | 30 | |||||
Dra | ο Dra | I/SB | 4,8 | 11,0 | – | – | 138,4 d | G9 III | 1,4 | 1,0 | CIA 8 | 18512+5923 | 96 | [113] (S, M) | ||
Dra | φ Dra | 1 (A/B) | V | 4,5 | 5,9 | 0,5″ | 2011 | 310 a | B9 IV + F8 IV | A3 IV | Σ 4,8 ± 0,5 | 2,7 ± 0,2 | STT 353 | 18208+7120 | 93 | [3] (UAa/Ab), [2] (S, M) |
2 (Aa/Ab) | SB | 4,5 | . | – | – | 26,8 d | B9 IV | F8 IV | 3,4 ± 0,3 | 1,4 ± 0,2 | ||||||
Dra | χ Dra | SI/SB | 3,7 | 5,7 | 0,1″ | 2009 | 281 d | F7 V | K0 V | 1,0 | 0,7 | LAB 5 | 18211+7244 | 8,3 | [33] (S, M, d) | |
Dra | ψ1 Dra | V | 4,6 | 5,6 | 29,6″ | 2019 | 10 000 a | F5 IV–V | F8 V | STF 2241 | 17419+7209 | 21 | ||||
Dra | ω Dra | SB/A | 4,8 | . | – | – | 5,28 d | F5 V | 1,5 | 1,2 | ome Dra | 17370+6845 | 24 | [88] (S, M) | ||
Dra | 17 / 16 Dra | 1 (17 = AB / 16 = C) | CPM | 5,0 | 5,5 | 90,2″ | 2018 | B8 V + A1 V | B9,5 V + DA1,6 | Σ 4,7 | STFA 30 | 16362+5255 | 130 | [24] (SA/B), [46] (SCa/Cb, MCa/Cb) | ||
2 (A/B) | V | 5,4 | 6,4 | 3,2″ | 2020 | B8 V | A1 V | STF 2078 | ||||||||
2 (Ca/Cb) | SB | 5,5 | . | – | – | B9,5 V | DA1,6 | 4,0 | 0,7 | |||||||
Dra | 20 Dra | V | 7,1 | 7,3 | 0,9″ | 2018 | 320 a | STF 2118 | 16564+6502 | 70 | ||||||
Dra | 26 Dra | 1 (AB/C) | CPM | 5,2 | 10,2 | 737,9″ | 2010 | F9 V + K3 V | M1 Ve | Σ 1,8 | LDS 2736 | 17350+6153 | 14 | [24] (SA/B), [18] (SC, M) | ||
2 (A/B) | V/SB | 5,3 | 8,5 | 0,6″ | 2013 | 76 a | F9 V | K3 V | 1,1 | 0,7 | BU 962 | |||||
Dra | 39 Dra | 1 (AB/C) | CPM | 5,0 | 8,0 | 88,9″ | 2017 | A0 V + F6 V | F7 IV | STF 2323 | 18239+5848 | 56 | [3] (UCa/Cb), [24] (SA/B) | |||
2 (A/B) | V | 5,1 | 8,1 | 3,8″ | 2019 | 2500 a | A0 V | F6 V | STF 2323 | |||||||
2 (Ca/Cb) | SB | 8,0 | . | – | – | 2,71 d | F7 IV | |||||||||
Dra | 41 / 40 Dra | 1 (41 = A / 40 = B) | V | 5,7 | 6,0 | 18,7″ | 2019 | 18 000 a | F7 V + F7 V | K2 V | Σ 2,5 ± 0,3 | STF 2308 | 18002+8000 | 45 | [3] (UBa/Bb), [114] (SAa/Ab, M) | |
2 (Aa/Ab) | SI/SB | 6,2 | 6,7 | 0,1″ | 2012 | 3,4 a | F7 V | F7 V | 1,3 ± 0,2 | 1,2 ± 0,2 | BAG 6 | |||||
2 (Ba/Bb) | SB | 5,6 | . | – | – | 10,5 d | K2 V | |||||||||
Dra | HR 6983 | 1 (AB/C) | CPM | 5,5 | 8,7 | 25,7″ | 2012 | K1 III + G9 III | F0 | STF 2348 | 18339+5221 | 200 | [24] (SA/B) | |||
2 (A/B) | V | 6,2 | 6,4 | 0,2″ | 2016 | 210 a | K1 III | G9 III | A 1377 | |||||||
Dra | Gliese 687 | SI | 9,2 | . | 0,3″ | 1993 | 24,5 a | M3 V | 0,4 | CHR 62 | 17364+6820 | 4,5 | [115] (M) | |||
Dra | Gliese 725 | V | 9,1 | 10,0 | 11,3″ | 2019 | 410 a | M3 V | M3,5 V | 0,3 | 0,3 | STF 2398 | 18428+5938 | 3,5 | [115] (M) | |
Equ | α Equ | I/SB | 3,9 | . | – | – | 98,8 d | G7 III | A4m | 2,1 | 1,0 | WRH 35 | 21158+0515 | 58 | [5] (S, M) | |
Equ | γ Equ | V | 4,7 | 8,7 | 0,6″ | 2014 | 270 a | A9 VpSrCrEu | K | 1,8 | 0,6 | KNT 5 | 21103+1008 | 35 | [116] (U, SB, M) | |
Equ | δ Equ | V/SB | 5,2 | 5,5 | 0,3″ | 2019 | 5,7 a | F7 V | F7 V | 1,2 | 1,2 | STT 535 | 21145+1000 | 18 | [33] (S, M, d) | |
Equ | ε Equ | 1 (AB/C) | V | 5,3 | 7,1 | 10,6″ | 2019 | F2 IV + F1 V + F7 IV | G0 V | Σ 5,1 ± 0,6 | STF 2737 | 20591+0418 | 54 | [3] (UAa/Ab), [24] (SB, SC), [2] (SAa/Ab, M) | ||
2 (A/B) | V | 6,0 | 6,3 | 0,0″ | 2020 | 104 a | F2 IV + F1 V | F7 IV | Σ 3,3 ± 0,4 | 1,8 | STF 2737 | |||||
3 (Aa/Ab) | SB | 6,0 | . | – | – | 2,03 d | F2 IV | F1 V | 1,8 | 1,5 | ||||||
Eri | θ Eri | V | 3,2 | 4,1 | 8,2″ | 2020 | A3 IV–V | A1 V | PZ 2 | 02583-4018 | 49 | |||||
Eri | ρ2 Eri | V | 5,4 | 8,9 | 1,4″ | 2002 | BU 11 | 03027-0741 | 74 | |||||||
Eri | τ4 Eri | V | 3,9 | 9,5 | 5,7″ | 2013 | JC 1 | 03195-2145 | 93 | |||||||
Eri | f Eri | V | 4,7 | 5,3 | 8,2″ | 2020 | B9,5 Van | A1 Va | DUN 16 | 03486-3737 | 51 | |||||
Eri | p Eri | V | 5,8 | 5,9 | 11,3″ | 2019 | 490 a | K0 V | K0 V | DUN 5 | 01398-5612 | 7,8 | [24] (S) | |||
Eri | 15 Eri | V | 6,6 | 5,3 | 0,2″ | 2018 | 118 a | SEE 23 | 03184-2231 | 78 | ||||||
Eri | 20 Eri | SI | 5,5 | 6,8 | 0,1″ | 2020 | 21,0 a | HDS 456 | 03363-1728 | 130 | ||||||
Eri | 32 Eri | V | 4,8 | 5,9 | 6,9″ | 2019 | G8 III | A1 V | STF 470 | 03543-0257 | 96 | |||||
Eri | 39 Eri | V | 5,0 | 8,5 | 6,4″ | 2015 | STF 516 | 04144-1015 | 69 | |||||||
Eri | 40 (ο2) Eri | 1 (A/BC) | CPM | 4,4 | 9,3 | 82,7″ | 2019 | K0 V | DA2,9 + M4,5 V | 0,8 | Σ 0,8 | STF 518 | 04153-0739 | 5,0 | [117] (MA), [118] (MB/C) | |
2 (B/C) | V | 9,5 | 11,2 | 8,2″ | 2019 | 223 a | DA2,9 | M4,5 V | 0,6 | 0,2 | STF 518 | |||||
Eri | 46 Eri | V | 5,7 | 9,2 | 1,3″ | 2009 | BU 881 | 04339-0644 | 270 | |||||||
Eri | 53 Eri | V | 4,0 | 7,0 | 1,1″ | 2016 | 77 a | KUI 18 | 04382-1418 | 36 | ||||||
Eri | 55 Eri | V | 6,7 | 6,8 | 9,3″ | 2018 | F2 VpSrSi | G5 III | STF 590 | 04436-0848 | 650 | |||||
Eri | 62 Eri | 1 (AB/C) | CPM | 5,5 | 11,4 | 127,1″ | 2011 | GMC 11 | 04564-0510 | 240 | ||||||
1 (A/B) | CPM | 5,5 | 8,9 | 66,1″ | 2013 | SHJ 48 | ||||||||||
2 (Aa/Ab) | SI | 5,5 | 9,6 | 0,4″ | 2015 | HDS 641 | ||||||||||
Eri | 63 Eri | SB/A | 5,5 | . | – | – | 2,5 a | K0 III–IV | D | 2,0 | 0,4 | 63 Eri | 04598-1016 | 53 | [119] (S, M) | |
For | α For | V | 4,0 | 7,2 | 5,4″ | 2017 | 270 a | F7 IV | G7 V | HJ 3555 | 03121-2859 | 14 | [24] (S) | |||
For | η2 For | V | 6,0 | 10,0 | 4,9″ | 2015 | HJ 3536 | 02502-3551 | 120 | |||||||
For | κ For | 1 (A/B) | SI/SB | 5,2 | 10,2 | 0,6″ | 2020 | 26,5 a | G1 V | M | 1,2 | Σ 1,0 | LAF 27 | 02225-2349 | 23 | [120] (UBa/Bb, S, M) |
2 (Ba/Bb) | SB | 10,2 | . | – | – | 3,67 d | M | M | 0,5 | 0,5 | ||||||
For | χ3 For | V | 6,5 | 10,1 | 6,5″ | 2015 | I 58 | 03282-3551 | 100 | |||||||
For | ω For | V | 5,0 | 7,7 | 11,0″ | 2013 | B9 Va | A5 V | HJ 3506 | 02338-2814 | 140 | |||||
Gem | α Gem (Kastor) | 1 (AB / C = YY Gem) | CPM | 1,6 | 9,8 | 69,8″ | 2017 | 13 000 a | A1 V + M5 V + A4 V + M0 V | M1 Ve + M1 Ve | 5,9 ± 0,4 | Σ 1,2 | STF 1110 | 07346+3153 | 16 | [3] (UAa/Ab, UBa/Bb), [121] (SAa/Ab, SBa/Bb, MAa/Ab, MBa/Bb), [33] (SCa/Cb, MCa/Cb) |
2 (A/B) | V | 1,9 | 3,0 | 5,4″ | 2020 | 460 a | A1 V + M5 V | A4 V + M0 V | 3,1 ± 0,2 | 2,8 ± 0,2 | STF 1110 | |||||
2 (Ca/Cb) | E/SB | 9,8 | . | – | – | 0,81 d | M1 Ve | M1 Ve | 0,6 | 0,6 | YY Gem | |||||
3 (Aa/Ab) | SB | 1,9 | . | – | – | 9,21 d | A1 V | M5 V | 2,7 | 0,4 | ||||||
3 (Ba/Bb) | SB | 3,0 | . | – | – | 2,93 d | A4 V | M0 V | 2,3 | 0,5 | ||||||
Gem | γ Gem (Alhena) | SI/SB | 1,9 | 7,5 | 0,4″ | 2012 | 12,6 a | A0 IVm | G | 2,8 | 1,1 | OCC 9011 | 06377+1624 | 34 | [122] (S, M) | |
Gem | δ Gem | 1 (A/B) | V | 3,6 | 8,2 | 5,5″ | 2018 | 1420 a | F1 IV–V | K3 V | STF 1066 | 07201+2159 | 19 | [24] (S) | ||
2 (Aa/Ab) | SB/A | 3,6 | . | – | – | 6,1 a | F1 IV–V | |||||||||
Gem | η Gem | 1 (A/B) | V | 3,5 | 6,2 | 1,7″ | 2018 | 1030 a | BU 1008 | 06149+2230 | 210 | [3] (UAa/Ab) | ||||
2 (Aa/Ab) | SB | 3,5 | . | – | – | 8,2 a | ||||||||||
Gem | κ Gem | V | 3,7 | 10,0 | 7,2″ | 2019 | STT 179 | 07444+2424 | 43 | |||||||
Gem | ν Gem | 1 (A/B) | SI | 4,1 | 5,1 | 0,1″ | 2020 | 19,1 a | B6 IVe | Be | Σ 5,2 ± 0,8 | 1,8 ± 0,4 | BTZ 1 | 06290+2013 | 170 | [106] (U, SB, M) |
2 (Aa/Ab) | A | 4,1 | . | – | – | 54,0 d | B6 IVe | 2,7 ± 0,4 | 2,5 ± 0,4 | |||||||
Gem | σ Gem | I/SB | 4,3 | 11,0 | – | – | 19,6 d | K1 III | 4,2 | ≥ 1,6 | CIA 7 | 07433+2853 | 38 | [111] (S, M) | ||
Gem | 1 Gem | 1 (A/B) | V/SB | 4,8 | 5,5 | 0,1″ | 2008 | 13,4 a | K0 III | F6 IV | 1,9 | Σ 2,7 | KUI 23 | 06041+2316 | 48 | [123] (UBa/Bb, S, M) |
2 (Ba/Bb) | SB/A | 5,5 | . | – | – | 9,60 d | F6 IV | G2 V | 1,7 | 1,0 | ||||||
Gem | 3 Gem | V | 5,9 | 8,5 | 0,6″ | 2008 | B2,5 Ib | 21 | BU 1241 | 06097+2307 | 2500 | [124] (S, M, d) | ||||
Gem | 4 Gem | V | 7,5 | 7,8 | 0,1″ | 2011 | 610 a | BU 1058 | 06105+2300 | 640 | ||||||
Gem | 38 Gem | V | 4,8 | 7,8 | 7,3″ | 2018 | 1750 a | A9 Vp | G6 V | STF 982 | 06546+1311 | 29 | [24] (S) | |||
Gem | 51 Gem | SI | 5,7 | 5,8 | 0,1″ | 1991 | HDS 1003 | 07134+1610 | 180 | |||||||
Gem | 63 Gem | 1 (A/B) | CPM | 5,2 | 11,0 | 43,0″ | 2006 | F1 V + F6 V + F5 V | Σ 3,6 | SHJ 368 | 07277+2127 | 34 | [125] (M), [2] (SAa1/Aa2), [60] (SAb, SD) | |||
2 (Aa/Ab) | SI | 5,3 | 7,3 | 0,1″ | 2018 | 2,1 a | F1 V + F6 V | F5 V | Σ 2,6 | 1,0 | MCA 30 | |||||
3 (Aa1/Aa2) | SB/A | 5,3 | . | – | – | 1,93 d | F1 V | F6 V | 1,4 | 1,2 | ||||||
Gem | 68 Gem | SI | 5,4 | 7,6 | 0,2″ | 2018 | 170 a | MCA 32 | 07336+1550 | 130 | ||||||
Gem | 82 Gem | SI | 6,9 | 7,3 | 0,3″ | 2016 | 580 a | K0 III | A0 IV: | WRH 15 | 07486+2308 | 240 | ||||
Gem | HR 2896 | 1 (A/B) | V | 6,1 | 6,5 | 0,1″ | 2015 | 210 a | K0 III | K + M: | 1,5 | Σ 1,5 | STT 175 | 07351+3058 | 110 | [125] (S, M) |
2 (Ba/Bb) | A | 6,5 | . | – | – | 2,0 a | K | M: | 1,3 | 0,2 | ||||||
Gru | θ Gru | 1 (AB/C) | CPM | 4,3 | 7,8 | 158,9″ | 2002 | JC 20 | 23069-4331 | 40 | ||||||
2 (A/B) | V | 4,5 | 6,6 | 1,5″ | 2013 | JC 20 | ||||||||||
Gru | ι Gru | SB/A | 3,9 | . | – | – | 1,1 a | iot Gru | 23104-4515 | 56 | ||||||
Gru | μ1 Gru | SI | 6,7 | 5,2 | 0,2″ | 2019 | 19,3 a | G8 III | G | 2,1 | 1,6 | CHR 187 | 22156-4121 | 74 | [13] (S), [27] (M) | |
Gru | υ Gru | V | 5,7 | 8,2 | 0,9″ | 2009 | BU 773 | 23069-3854 | 87 | |||||||
Her | α Her (Ras Algethi) | 1 (α1 = A / α2 = B) | V | 3,5 | 5,4 | 4,7″ | 2020 | 3600 a | M5 Ib–II | G8 III + A9 IV–V | 2,1–3,3 | Σ 3,7–5,3 | STF 2140 | 17146+1423 | 110 | [3] (UBa/Bb), [126] (S, M) |
2 (Ba/Bb) | SB | 5,4 | . | – | – | 51,6 d | G8 III | A9 IV–V | 2,1–3,0 | 1,6–2,3 | ||||||
Her | β Her | I/SB | 2,8 | . | – | – | 1,1 a | 2,9 | 0,9 | BLA 4 | 16302+2129 | 43 | [127] (M) | |||
Her | δ Her | - (A/B) | O | 3,1 | 8,3 | 13,7″ | 2019 | A1 Vn | G4 IV–V | STF 3127 | 17150+2450 | 23 | ||||
1 (Aa/Ab) | SI | 3,1 | 4,4 | 0,1″ | 1989 | BNU 5 | 17150+2450 | 320 | ||||||||
Her | ζ Her | V | 3,0 | 5,4 | 1,6″ | 2019 | 34,5 a | F9 IV | G7 V | 1,5 | 1,0 | STF 2084 | 16413+3136 | 10,7 | [24] (S), [128] (M) | |
Her | κ Her | V | 5,1 | 6,2 | 27,0″ | 2019 | G7 III | K0 IV | STF 2010 | 16081+1703 | 120 | |||||
Her | μ Her | 1 (μ1 = A / μ2 = BC) | CPM | 3,5 | 9,8 | 35,5″ | 2015 | G5 IV + M4 | M3 + M4 | Σ 1,4 | Σ 0,8 | STF 2220 | 17465+2743 | 8,3 | [40] (SB/C), [129] (SAa/Ab, MAa/Ab), [130] (MB/C) | |
2 (Aa/Ab) | V(IR) | 3,5 | 12,7 | 1,8″ | 2015 | 99 a | G5 IV | M4 | 1,1 | 0,3 | TRN 2 | |||||
2 (B/C) | V | 10,2 | 10,7 | 0,8″ | 2015 | 43 a | M3 | M4 | 0,4 | 0,4 | AC 7 | |||||
Her | ν Her | SI | 4,6 | 7,5 | 0,5″ | 1996 | HDS 2534 | 17585+3011 | 260 | |||||||
Her | ρ Her | 1 (A/B) | V | 4,5 | 5,4 | 4,1″ | 2019 | A0 III | B9,5 IVn | STF 2161 | 17237+3709 | 120 | ||||
2 (Aa/Ab) | SI | 4,9 | 5,9 | 0,3″ | 2018 | A0 III | MCA 48 | |||||||||
Her | σ Her | SI | 4,2 | 7,7 | 0,1″ | 2008 | 7,4 a | B7 | A9 | 3,9 | 1,8 | LAB 4 | 16341+4226 | 77 | [11] (S, M) | |
Her | φ Her | I/SB | 4,2 | . | – | – | 1,5 a | B9:p(HgMn) | 3,1 | 1,6 | NOI 2 | 16088+4456 | 67 | [131] (S, M) | ||
Her | c Her | V | 6,1 | 6,1 | 0,1″ | 2018 | 8,1 a | A9 III–IV | A9 III–IV | Σ 3,3 ± 0,4 | HU 1176 | 17080+3556 | 56 | [24] (S), [9] (M) | ||
Her | 25 Her | SI | 5,6 | 8,3 | 0,1″ | 2007 | 76 a | CHR 55 | 16254+3724 | 77 | ||||||
Her | 52 Her | 1 (A/BC) | V | 4,8 | 8,5 | 2,2″ | 2018 | 870 a | A1 VpSiSrCr | K–M + K–M | 2,2 ± 0,2 | Σ 1,2 | BU 627 | 16492+4559 | 55 | [58] (SB/C, MB/C), [132] (MA) |
2 (B/C) | V(aO) | 9,5 | 9,6 | 0,3″ | 2012 | 56 a | K–M | K–M | Σ 1,2 | A 1866 | ||||||
Her | 79 Her | SI | 5,9 | 7,3 | 0,1″ | 2008 | 10,4 a | A1 V | A8 V | Σ 3,1 | CHR 63 | 17375+2419 | 78 | [38] (S, M) | ||
Her | 90 Her | V | 5,3 | 8,8 | 1,6″ | 2009 | BU 130 | 17533+4000 | 110 | |||||||
Her | 95 Her | V | 4,9 | 5,2 | 6,4″ | 2019 | A5 IIIn | G5 III | STF 2264 | 18015+2136 | 130 | |||||
Her | 99 Her | V | 5,1 | 9,0 | 1,4″ | 2018 | 56 a | F7 V | K4 V | 0,9 | 0,5 | AC 15 | 18070+3034 | 16 | [133] (S, M) | |
Her | 100 Her | 1 (A/B) | V | 5,8 | 5,8 | 14,3″ | 2019 | A3 V | A3 V | STF 2280 | 18078+2606 | 63 | ||||
2 (Aa/Ab) | SI | 5,9 | 8,8 | 0,0″ | 2019 | 36 a | A3 V | CHR 67 | ||||||||
Her | 113 Her | I/SB | 4,8 | 6,8 | – | – | 246 d | G7 II | A0 V | 3,2 | 2,2 | MKT 9 | 18547+2239 | 130 | [5] (S, M) | |
Her | 49 Ser | V | 7,4 | 7,5 | 4,0″ | 2019 | 950 a | G8 V | G8 V | STF 2021 | 16133+1332 | 24 | [24] (S) | |||
Her | V772 Her | 1 (AB/C) | V | 7,2 | 10,6 | 28,2″ | 2015 | G1 V + K6 V + G8 V | K7 V + M0 V | STT 341 | 18058+2127 | 33 | [3] (UAa/Ab, UCa/Cb), [21] (SAa/Ab, SCa/Cb) | |||
2 (A/B) | V/SB | 7,4 | 8,8 | 0,1″ | 2019 | 20,1 a | G1 V + K6 V | G8 V | STT 341 | |||||||
2 (Ca/Cb) | SB | 10,6 | . | – | – | 25,8 d | K7 V | M0 V | ||||||||
3 (Aa/Ab) | E/SB | 7,4 | . | – | – | 0,88 d | G1 V | K6 V | ||||||||
Her | V819 Her | 1 (A/B) | SI | 6,1 | 6,4 | 0,1″ | 2017 | 5,5 a | G7 III–IV | F2 V + F8 V | 1,8 | Σ 2,6 | MCA 47 | 17217+3958 | 71 | [21] (UBa/Bb, S), [134] (M) |
2 (Ba/Bb) | E/SB | 6,4 | . | – | – | 2,23 d | F2 V | F8 V | 1,5 | 1,1 | ||||||
Her | HR 6594 | V | 5,6 | 9,4 | 1,4″ | 2016 | 144 a | BU 1251 | 17420+1557 | 35 | ||||||
Her | HR 6627 | V | 6,0 | 6,9 | 0,4″ | 2018 | 1060 a | B9 | A2 | 3,0 | 2,3 | STF 2215 | 17471+1742 | 140 | [11] (S, M) | |
Her | HR 6980 | V | 6,4 | 6,6 | 0,7″ | 2019 | 220 a | G9 III | G7 III | STT 359 | 18355+2336 | 140 | [24] (S) | |||
Her | Furuhjelm 46 | V | 10,0 | 10,3 | 0,3″ | 2016 | 13,0 a | M3 | M3,5 | 0,4 | 0,4 | KUI 79 | 17121+4540 | 6,0 | [40] (S), [112] (M) | |
Her | DQ Her | E | 14,4 | . | – | – | 0,19 d | M3 Ve | D | 0,4 | 0,6 | 500 | [30] (V), [135] (U, S2, M) | |||
Hor | δ Hor | SI | 5,2 | 7,3 | 0,1″ | 2019 | HDS 530 | 04108-4200 | 55 | |||||||
Hor | η Hor | SI | 5,5 | 6,5 | 0,1″ | 2020 | 3,2 a | A6 V | F0 V | TOK 186 | 02374-5233 | 42 | [136] (S) | |||
Hya | β Hya | V | 4,7 | 5,5 | 0,6″ | 2015 | HJ 4478 | 11529-3354 | 95 | |||||||
Hya | ε Hya | 1 (ABC/D) | V | 3,4 | 12,5 | 18,1″ | 2017 | G5 III + A8 IV + dF7 | STF 1273 | 08468+0625 | 40 | [3] (UCa/Cb), [13] (S) | ||||
2 (AB/C) | V | 3,5 | 6,7 | 2,9″ | 2020 | 370 a | G5 III + A8 IV | dF7 | STF 1273 | |||||||
3 (A/B) | V/SB | 3,5 | 5,0 | 0,2″ | 2018 | 15,1 a | G5 III | A8 IV | SP 1 | |||||||
3 (Ca/Cb) | SB | 6,7 | . | – | – | 9,90 d | dF7 | |||||||||
Hya | λ Hya | SB/A | 3,6 | . | – | – | 4,3 a | lam Hya | 10106-1221 | 33 | ||||||
Hya | χ1 Hya | SI | 5,7 | 5,7 | 0,1″ | 2020 | 7,6 a | F4 V | F4 V | Σ 3,9 ± 0,6 | FIN 47 | 11053-2718 | 44 | [24] (S), [53] (M) | ||
Hya | χ2 Hya | E/SB | 5,7 | . | – | – | 2,27 d | B8 V | B8 V | 3,6 | 2,6 | 220 | [30] (V), [33] (U, S, M, d) | |||
Hya | 15 Hya | 1 (A/B) | V | 5,8 | 7,4 | 1,2″ | 2017 | BU 587 | 08516-0711 | 140 | [3] (U) | |||||
2 (Aa/Ab) | SB | 5,8 | . | – | – | 2,90 d | ||||||||||
Hya | 17 Hya | V | 6,7 | 6,9 | 4,0″ | 2020 | kA4hF1mF2 | kA1hF2mF3 | STF 1295 | 08555-0758 | 88 | |||||
Hya | 19 Hya | V | 5,6 | 9,5 | 1,3″ | 2006 | KUI 38 | 09087-0835 | 320 | |||||||
Hya | 23 Hya | 1 (A/B) | V | 5,3 | 10,8 | 1,6″ | 2019 | KUI 40 | 09167-0621 | 100 | [3] (U) | |||||
2 (Aa/Ab) | SB/A | 5,3 | . | – | – | 2,5 a | ||||||||||
Hya | 29 Hya | 1 (AB/C) | V | 6,5 | 11,3 | 10,9″ | 2019 | A 1588 | 09272-0913 | 230 | ||||||
2 (A/B) | V | 7,0 | 7,8 | 0,4″ | 2011 | BU 590 | ||||||||||
Hya | 52 Hya | 1 (AB/C) | V | 5,0 | 10,0 | 2,4″ | 2010 | BU 940 | 14282-2929 | 120 | ||||||
2 (A/B) | SI | 5,7 | 5,7 | 0,1″ | 1989 | FIN 306 | ||||||||||
Hya | 54 Hya | V | 5,1 | 7,3 | 8,1″ | 2015 | F0 VSr | G1 V | H 3 97 | 14460-2527 | 30 | |||||
Hya | 59 Hya | V | 6,2 | 6,8 | 0,5″ | 2019 | 430 a | A4 V | A6 V | BU 239 | 14587-2739 | 110 | [24] (S) | |||
Hya | 17 Crt | V | 5,6 | 5,7 | 9,6″ | 2015 | F8 V | F8 V | H 3 96 | 11323-2916 | 26 | |||||
Hya | HR 5120 | V | 5,7 | 6,6 | 10,2″ | 2015 | A7 III–IV | F0 Vn | H N 69 | 13368-2630 | 100 | |||||
Hyi | α Hyi | A | 2,9 | . | – | – | 1,7 a | F0 IV | alp Hyi | 01588-6134 | 22 | |||||
Ind | δ Ind | SI | 4,8 | 6,0 | 0,1″ | 2020 | 12,2 a | A8 IV | G0–7 IV | 1,8 ± 0,3 | 1,3 ± 0,2 | FIN 307 | 21579-5500 | 58 | [16] (S, M) | |
Ind | ε Ind | 1 (A/B) | CPM | 4,8 | 24,0 | 403,1″ | 2010 | K5 V | T1 + T6 | 0,8 | Σ 0,12 | SOZ 1 | 22034-5647 | 3,6 | [137] (SA, MA), [138] (SBa/Bb, MBa/Bb) | |
2 (Ba/Bb) | V(aO) | 24,1 | > 26,6 | 0,9″ | 2005 | 11,2 a | T1 | T6 | 0,07 | 0,05 | VLK 1 | |||||
Ind | θ Ind | 1 (A/B) | V | 4,5 | 6,9 | 7,3″ | 2015 | A5 IV–V + A5 V | G0V | HJ 5258 | 21199-5327 | 30 | [136] (UAa/Ab, SAb) | |||
2 (Aa/Ab) | I | 4,9 | 5,1 | – | – | ≈ 1,3 a | A5 IV–V | A5 V | MRN 3 | |||||||
Lac | 8 Lac | 1 (A/B) | O? | 5,7 | 6,3 | 22,3″ | 2018 | B1 IVe | B1,5 Vs | STF 2922 | 22359+3938 | 550 | ||||
2 (Aa/Ab) | SI | 5,7 | . | 0,0″ | 2018 | 42 a | CHR 112 | |||||||||
Leo | α Leo (Regulus) | 1 (A/BC) | CPM | 1,4 | 8,2 | 179,2″ | 2019 | B7 V + D | K2 V + M4 V | Σ 4,0 ± 1,5 | Σ ≈ 1,0 | STFB 6 | 10084+1158 | 24 | [139] (UAa/Ab), [140] (MAa/Ab), [141] (S, MB/C) | |
2 (Aa/Ab) | SB | 1,4 | . | – | – | 40,1 d | B7 V | D | 3,7 ± 1,4 | 0,3 ± 0,1 | ||||||
2 (B/C) | V | 8,2 | 13,2 | 2,2″ | 2019 | K2 V | M4 V | ≈ 0,8 | ≈ 0,2 | HDO 127 | ||||||
Leo | γ Leo (Algieba) | V | 2,4 | 3,6 | 4,7″ | 2020 | 550 a | K1 III | G7 IIIb | STF 1424 | 10200+1950 | 40 | ||||
Leo | η Leo | SI | 3,5 | 8,4 | 0,4″ | 2015 | WRH 18 | 10073+1646 | 390 | |||||||
Leo | ι Leo | V | 4,1 | 6,7 | 2,2″ | 2019 | 184 a | F1 IV | G3 V | 1,6–1,7 | STF 1536 | 11239+1032 | 24 | [24] (S), [142] (M) | ||
Leo | κ Leo | V | 4,6 | 9,7 | 2,0″ | 2015 | BU 105 | 09247+2611 | 62 | |||||||
Leo | ο Leo | I/SB | 3,5 | . | – | – | 14,5 d | F8 IIIm | A7m | 2,1 | 1,9 | HMM 1 | 09412+0954 | 40 | [5] (S, M) | |
Leo | χ Leo | V | 4,7 | 11,0 | 4,9″ | 2018 | KUI 54 | 11050+0720 | 29 | |||||||
Leo | ω Leo | V/SB | 5,7 | 7,3 | 0,9″ | 2019 | 118 a | G1 V | 1,9 ± 1,0 | 0,3 ± 0,9 | STF 1356 | 09285+0903 | 33 | [9] (M) | ||
Leo | 19 Leo | SI | 6,4 | 6,9 | 0,1″ | 2019 | 15,2 a | MCA 34 | 09474+1134 | 85 | ||||||
Leo | 49 Leo | 1 (A/B) | V | 5,8 | 7,9 | 2,0″ | 2019 | A2 V | B | STF 1450 | 10350+0839 | 130 | [21] (U, S) | |||
2 (Aa/Ab) | E/SB | 5,8 | . | – | – | 2,45 d | ||||||||||
Leo | 54 Leo | V | 4,5 | 6,3 | 6,8″ | 2019 | A1 V | A2 Vn | STF 1487 | 10556+2445 | 88 | |||||
Leo | 55 Leo | V | 6,0 | 9,0 | 1,1″ | 2019 | 139 a | BU 1076 | 10557+0044 | 46 | ||||||
Leo | 65 Leo | V | 5,7 | 9,7 | 2,8″ | 2015 | BU 599 | 11069+0157 | 61 | |||||||
Leo | 73 Leo | SI/SB | 5,5 | 7,3 | 0,1″ | 2020 | 8,1 a | MCA 35 | 11159+1318 | 110 | ||||||
Leo | 83 Leo | V | 6,6 | 7,5 | 28,6″ | 2019 | 32 000 a | K0 IV | K2 IV–V | STF 1540 | 11268+0301 | 18 | [24] (S) | |||
Leo | 88 Leo | V | 6,3 | 9,1 | 15,7″ | 2020 | 3500 a | F9,5 V | K5 | STF 1547 | 11317+1422 | 24 | ||||
Leo | 90 Leo | V | 6,3 | 7,3 | 3,1″ | 2018 | B6,6 IV | B3,7 V | STF 1552 | 11347+1648 | 580 | |||||
Leo | 93 Leo | 1 (A/B) | CPM | 4,6 | 9,0 | 75,5″ | 2020 | G7 III + A7 IV | G5 | Σ 4,2 ± 0,3 | STFB 7 | 11480+2013 | 71 | [143] (SAa/Ab, M) | ||
2 (Aa/Ab) | I/SB | 5,1 | 5,6 | – | – | 71,7 d | G7 III | A7 IV | 2,2 ± 0,2 | 2,0 ± 0,2 | MKT 7 | |||||
Leo | HR 4465 | V | 6,4 | 6,8 | 0,7″ | 2019 | 1730 a | STF 1555 | 11363+2747 | 72 | ||||||
Lep | β Lep | V | 2,9 | 7,5 | 2,7″ | 2017 | BU 320 | 05282-2046 | 49 | |||||||
Lep | ι Lep | V | 4,5 | 9,9 | 11,9″ | 2015 | B7,5 Vn | G8 Ve | STF 655 | 05123-1152 | 71 | |||||
Lep | κ Lep | V | 4,4 | 6,8 | 2,2″ | 2008 | STF 661 | 05132-1256 | 220 | |||||||
Lep | HR 1771 | V | 5,4 | 6,6 | 3,5″ | 2015 | G8–K0 II–III | A2–3 | HJ 3752 | 05218-2446 | 110 | |||||
Lep | Gliese 229 | V(IR) | 8,4 | 17,1 | 6,2″ | 2011 | M1 V | T6,5 | 0,7 | 0,03–0,04 | NAJ 1 | 06106-2152 | 5,8 | [115] (M1), [144] (M2) | ||
Lib | α Lib (Zuben-el-dschenubi) | 1 (α2/1 = AB / D = KU Lib) | CPM | 2,7 | 7,3 | 2,6° | – | A4 IV–V + F: + F4 V + M: | G8 V (k) | Σ ≈ 5,7 | ≈ 1,0 | CAB 1 | 14509-1603 | 23 | [145] (ρAB/D, UBa/Bb, S, M), [146] (UAa/Ab) | |
2 (α2 = A / α1 = B) | CPM | 2,7 | 5,2 | 231,1″ | 2012 | A4 IV–V + F: | F4 V + M: | Σ ≈ 3,7 | Σ ≈ 2,0 | SHJ 186 | ||||||
3 (Aa/Ab) | SB | 3,3 | 3,7 | – | – | 70,3 d | A4 IV–V | F: | ≈ 2,2 | ≈ 1,5 | DSG 17 | |||||
3 (Ba/Bb) | V(aO)/SB | 5,2 | . | 0,2″ | 2018 | 16,1 a | F4 V | M: | ≈ 1,4–1,5 | ≈ 0,5–0,6 | BEU 19 | |||||
Lib | ι Lib | 1 (A/BC) | CPM | 4,5 | 10,9 | 57,8″ | 2013 | B8 VpSi + B9 IV–V | G5 IV | Σ 6,1 ± 2,3 | H 6 44 | 15122-1948 | 120 | [13] (S), [53] (M) | ||
2 (Aa/Ab) | V/SB | 5,1 | 5,5 | 0,1″ | 2019 | 23,5 a | B8 VpSi | B9 IV–V | Σ 6,1 ± 2,3 | B 2351 | ||||||
2 (B/C) | V | 10,9 | 11,4 | 2,4″ | 2015 | G5 IV | BU 618 | |||||||||
Lib | μ Lib | V | 5,6 | 6,6 | 1,9″ | 2019 | 610 a | BU 106 | 14493-1409 | 73 | ||||||
Lib | υ Lib | V | 3,6 | 10,8 | 2,0″ | 2002 | I 1271 | 15370-2808 | 69 | |||||||
Lib | 5 Lib | V | 6,5 | 10,1 | 4,7″ | 2001 | HLD 20 | 14460-1528 | 170 | |||||||
Lib | 18 Lib | V | 6,0 | 9,8 | 19,6″ | 2013 | STF 1894 | 14589-1109 | 110 | |||||||
Lib | 47 Lib | V | 6,0 | 8,5 | 0,4″ | 2018 | 360 a | HU 1274 | 15550-1923 | 240 | ||||||
Lib | Gliese 570 | 1 (AB/D) | CPM | 5,8 | 13,9 | 259,8″ | 1998 | K4 V + M1,5 V + M3 V | T7,5 | Σ 1,6 | ≈ 0,03 | H N 28 | 14575-2125 | 6,5 | [1] (MBa/Bb, d), [2] (SA, SBa/Bb, MA), [147] (SD, MD) | |
2 (A/B) | V | 5,9 | 8,2 | 26,2″ | 2020 | 6500 a | K4 V | M1,5 V + M3 V | 0,7 | Σ 0,9 | H N 28 | |||||
3 (Ba/Bb) | I/SB | 8,2 | 9,8 | – | – | 309 d | M1,5 V | M3 V | 0,5 | 0,4 | ||||||
LMi | β LMi | V/SB | 4,6 | 6,0 | 0,5″ | 2018 | 38,2 a | K0 III–IV | F8 V | HU 879 | 10279+3642 | 47 | [24] (S) | |||
LMi | 11 LMi | V | 4,8 | 12,5 | 6,7″ | 2012 | 240 a | G8 Va | M5 V | HU 1128 | 09357+3549 | 11,2 | ||||
Lup | γ Lup | 1 (A/B) | V | 3,0 | 4,5 | 0,8″ | 2020 | 190 a | B1 V + B2 V | B3 V | 20 | 7 | HJ 4786 | 15351-4110 | 130 | [3] (UAa/Ab), [2] (S, M) |
2 (Aa/Ab) | SB | 4,5 | . | – | – | 2,81 d | B1 V | B2 V | 12 | 8 | ||||||
Lup | ε Lup | 1 (A/B) | V | 3,6 | 5,0 | 0,1″ | 2019 | 740 a | COP 2 | 15227-4441 | 160 | [3] (UAa/Ab) | ||||
2 (Aa/Ab) | SB | 3,6 | . | – | – | 4,56 d | ||||||||||
Lup | ζ Lup | CPM | 3,5 | 6,7 | 71,7″ | 2020 | G8 III | F6 V | DUN 176 | 15123-5206 | 36 | |||||
Lup | η Lup | V | 3,4 | 7,5 | 14,8″ | 2020 | RMK 21 | 16001-3824 | 140 | |||||||
Lup | κ Lup | V | 3,8 | 5,5 | 26,3″ | 2020 | B9,5 Vne | A3–5 V | DUN 177 | 15119-4844 | 54 | |||||
Lup | λ Lup | V | 4,4 | 5,2 | 0,1″ | 2019 | 71 a | B3 V | B3 V | 8,1 | 5,8 | SEE 219 | 15088-4517 | 170 | [24] (S), [68] (M, d) | |
Lup | μ Lup | 1 (AB/C) | V | 4,2 | 6,3 | 23,1″ | 2019 | B7 V + B7 V | A2–3 V | DUN 180 | 15185-4753 | 100 | ||||
2 (A/B) | V | 4,9 | 5,0 | 0,7″ | 2019 | 770 a | B7 V | B7 V | HJ 4753 | |||||||
Lup | ξ Lup | V | 5,1 | 5,6 | 10,2″ | 2020 | A3 V | B9 V | PZ 4 | 15569-3358 | 65 | |||||
Lup | ο Lup | SI | 5,3 | 4,8 | 0,0″ | 2020 | 33 a | FIN 319 | 14516-4335 | 120 | ||||||
Lup | π Lup | V | 4,6 | 4,6 | 1,6″ | 2019 | B5 IV | B5 V | HJ 4728 | 15051-4703 | 150 | |||||
Lup | τ2 Lup | V | 4,9 | 5,6 | 0,1″ | 2020 | 26,0 a | F4 IV | A7: | I 402 | 14262-4523 | 98 | [13] (S) | |||
Lup | υ Lup | V | 5,4 | 10,9 | 1,6″ | 2015 | RST 1839 | 15248-3943 | 120 | |||||||
Lup | d Lup | V | 4,7 | 6,5 | 2,1″ | 2016 | HJ 4788 | 15359-4457 | 130 | |||||||
Lyn | 4 Lyn | V | 6,1 | 7,7 | 0,6″ | 2016 | 500 a | STF 881 | 06221+5922 | 150 | ||||||
Lyn | 12 Lyn | 1 (AB/C) | V | 5,4 | 7,1 | 8,9″ | 2019 | A1,5 V + A2 V | kA6hF1mF1 | STF 948 | 06462+5927 | 66 | ||||
2 (A/B) | V | 5,4 | 6,0 | 1,9″ | 2019 | 730 a | A1,5 V | A2 V | STF 948 | |||||||
Lyn | 14 Lyn | V | 6,0 | 6,5 | 0,3″ | 2015 | 320 a | STF 963 | 06531+5927 | 150 | ||||||
Lyn | 15 Lyn | V | 4,5 | 5,5 | 0,7″ | 2017 | 260 a | STT 159 | 06573+5825 | 55 | ||||||
Lyn | 19 Lyn | 1 (AB/D) | CPM | 5,4 | 7,6 | 215,3″ | 2002 | B8 V + B9 V | A0 V | STF 1062 | 07229+5517 | 210 | ||||
2 (A/B) | V | 5,8 | 6,7 | 13,8″ | 2019 | B8 V | B9 V | STF 1062 | ||||||||
Lyn | 20 Lyn | V | 7,5 | 7,7 | 14,9″ | 2017 | A8 V | A6 V | STF 1065 | 07223+5009 | 160 | |||||
Lyn | 38 Lyn | 1 (A/B) | V | 3,9 | 6,1 | 2,6″ | 2019 | 2800 a | A1 V | A4 V | STF 1334 | 09188+3648 | 38 | |||
2 (Ba/Bb) | SI | 6,1 | . | 0,2″ | 2004 | CHR 173 | ||||||||||
Lyn | 10 UMa | V/SB | 4,2 | 6,5 | 0,4″ | 2017 | 21,8 a | F3 V | K0 V | 1,4 | 0,9 | KUI 37 | 09006+4147 | 16 | [148] (S, M) | |
Lyn | HR 2486 | V | 6,3 | 6,3 | 4,5″ | 2019 | 2000 a | F6 V | F4 V | STF 958 | 06482+5542 | 43 | ||||
Lyr | β Lyr | 1 (A/B) | CPM | 3,4 | 6,7 | 45,7″ | 2017 | B6–8 II + B | B7 V | Σ 16 | STFA 39 | 18501+3322 | 310 | [149] (SAa1/Aa2, M, d) | ||
2 (Aa1/Aa2) | E/I/SB | 3,6 | 4,0 | – | – | 12,9 d | B6–8 II | B | 13 | 3 | CIA 3 | |||||
Lyr | ε Lyr | 1 (ε1 = AB / ε2 = CD) | CPM | 4,7 | 4,6 | 209,5″ | 2016 | ≈ 340 000 a | A3 V + F0 V | A6 Vn + A7 Vn | Σ 3,9 | Σ 3,6 | STFA 37 | 18443+3940 | 50 | [150] (UAB/CD, M) |
2 (A/B) | V | 5,2 | 6,1 | 2,2″ | 2020 | 2800 a | A3 V | F0 V | 2,3 | 1,6 | STF 2382 | |||||
2 (C/D) | V | 5,3 | 5,4 | 2,4″ | 2020 | 720 a | A6 Vn | A7 Vn | 1,9 | 1,7 | STF 2383 | |||||
Lyr | ζ Lyr | 1 (ζ1 = A / ζ2 = D) | CPM | 4,3 | 5,6 | 43,7″ | 2018 | kA5hF0VmF3 | F1 Vnn | STFA 38 | 18448+3736 | 48 | [3] (U) | |||
2 (Aa/Ab) | SB | 4,3 | . | – | – | 4,3 d | ||||||||||
Lyr | η Lyr | 1 (A/B) | O? | 4,4 | 8,6 | 28,4″ | 2017 | B2,5 IV | A0 IVn | STF 2487 | 19138+3909 | 430 | [3] (U) | |||
2 (Aa/Ab) | SB | 4,4 | . | – | – | 56,4 d | B2,5 IV | |||||||||
Lyr | ι Lyr | SI | 5,3 | 6,4 | 0,1″ | 2014 | 220 a | STA 3 | 19073+3606 | 280 | ||||||
Lyr | HR 7162 | V | 5,3 | 8,0 | 1,3″ | 2015 | 63 a | F9 V | K1 V | 1,1 | 0,7 | BU 648 | 18570+3254 | 15 | [36] (M) | |
Lyr | GJ 758 | V(aO) | 4,8 | . | 1,6″ | 2017 | 96 a | G8 V | T7 | 1,0 | 0,04–0,05 | THA 1 | 19236+3313 | 16 | [151] (S, M) | |
Lyr | 17 Lyr | 1 (A/B) | V | 5,3 | 9,1 | 3,2″ | 2017 | > 1200 a | F0 V | G: | ≈ 1,8 | ≈ 0,8 | STF 2461 | 19074+3230 | 44 | [152] (UA/B, S, M), [3] (UAa/Ab) |
2 (Aa/Ab) | SB | 5,3 | . | – | – | 42,9 d | F0 V | |||||||||
Mic | α Mic | O? | 5,0 | 10,1 | 20,2″ | 2010 | HJ 5224 | 20500-3347 | 120 | |||||||
Mic | θ2 Mic | V | 6,2 | 6,9 | 0,3″ | 2019 | 460 a | BU 766 | 21244-4100 | 120 | ||||||
Mon | β Mon | 1 (β1/2 = AB / C) | V | 4,0 | 5,4 | 9,9″ | 2019 | B4 Ve(shell) + B2 Vn(e) | B3 V:nne | STF 919 | 06288-0702 | 210 | ||||
1 (β1 = A / β2 = B) | V | 4,6 | 5,0 | 7,1″ | 2019 | B4 Ve(shell) | B2 Vn(e) | STF 919 | ||||||||
Mon | ε Mon | V | 4,4 | 6,6 | 12,2″ | 2019 | A7 IV | F4 V | STF 900 | 06238+0436 | 41 | |||||
Mon | 3 Mon | V | 5,0 | 8,0 | 1,9″ | 1996 | BU 16 | 06018-1036 | 220 | |||||||
Mon | 14 Mon | V | 6,5 | 10,6 | 11,0″ | 2012 | STF 938 | 06348+0734 | 200 | |||||||
Mon | 15 Mon | 1 (A/B) | O? | 4,6 | 7,8 | 3,0″ | 2018 | O7 V((f))z | B2 | Σ 45 ± 4 | STF 950 | 06410+0954 | 720 | [153] (U, S, M, d) | ||
2 (Aa/Ab) | SI/SB | 4,7 | 5,9 | 0,1″ | 2018 | 108 a | O7 V((f))z | Σ 45 ± 4 | CHR 168 | |||||||
Mon | Ross 614 | V | 11,0 | 14,8 | 1,3″ | 2020 | 16,6 a | M4 V | M5,5 V | 0,2 | 0,11 | B 2601 | 06293-0248 | 4,1 | [154] (S), [155] (M) | |
Mon | WISE 0720−0846 (Scholz’ Stern) | V(aO) | 18,3 | . | 0,4″ | 2019 | 8,1 a | M9,5 | T5,5 | 0,09 | 0,06 | BUG 17 | 07200-0847 | 6,8 | [156] (V) [157] (U, S, M, d) | |
Mus | β Mus | V | 3,5 | 4,0 | 1,0″ | 2019 | 460 a | B2 V | B3 V | R 207 | 12463-6806 | 100 | [24] (S) | |||
Mus | δ Mus | SB/A | 3,6 | . | – | – | 1,2 a | del Mus | 13023-7133 | 28 | ||||||
Mus | η Mus | 1 (AB/C) | CPM | 4,8 | 7,2 | 58,2″ | 2015 | B7 III | B7 III | DUN 131 | 13152-6754 | 120 | [3] (U) | |||
2 (A/B) | V(IR) | 4,8 | . | 2,5″ | 2015 | B7 III | HUB 11 | |||||||||
3 (Aa/Ab) | SB | 4,8 | . | – | – | 20,0 d | B7 III | |||||||||
Mus | θ Mus | 1 (A/B) | V | 5,7 | 7,6 | 5,5″ | 2016 | WC5–6 + O6–7 V + O9,5–B0 Iab | O9 III | RMK 16 | 13081-6518 | 2300 | [158] (SAa1/Aa2, UAa1/Aa2, d) | |||
2 (Aa/Ab) | SI | 5,9 | 6,6 | 0,0″ | 2016 | WC5–6 + O6–7 V | O9,5–B0 Iab | CHR 247 | ||||||||
3 (Aa1/Aa2) | SB | 5,9 | . | – | – | 19,1 d | WC5–6 | O6–7 V | ||||||||
Mus | λ Mus | A | 3,6 | . | – | – | 1,2 a | lam Mus | 11456-6644 | 39 | ||||||
Mus | 12 G. Mus | 1 (A/B) | V | 5,5 | 6,6 | 0,2″ | 2018 | 97 a | K4 III + dF–G | A0 V + A2 V | B 1705 | 11395-6524 | 150 | [21] (UAa/Ab, UBa/Bb, S) | ||
2 (Aa/Ab) | SB | 5,5 | . | – | – | 61 d | K4 III | dF–G | ||||||||
2 (Ba/Bb) | E/SB | 6,6 | . | – | – | 2,75 d | A0 V | A2 V | ||||||||
Mus | HR 4401 | V | 5,4 | 6,6 | 2,5″ | 2016 | B5 IV | B9,5 IV | HJ 4432 | 11234-6457 | 120 | |||||
Nor | ε Nor | 1 (A/B) | V | 4,5 | 6,1 | 22,9″ | 2016 | B3 V + B3 V | A | HJ 4853 | 16272-4733 | 160 | [159] (U, SAa/Ab) | |||
2 (Aa/Ab) | SB | 4,5 | . | – | – | 3,26 d | B3 V | B3 V | ||||||||
Nor | ι1 Nor | 1 (AB/C) | V | 4,6 | 8,0 | 11,0″ | 2019 | A5 V + A6 V | HJ 4825 | 16035-5747 | 39 | [13] (S) | ||||
2 (A/B) | V | 5,2 | 5,8 | 0,2″ | 2020 | 26,8 a | A5 V | A6 V | SEE 258 | |||||||
Nor | λ Nor | V | 5,8 | 6,9 | 0,4″ | 2018 | 68 a | A4 | A7 | SEE 271 | 16193-4240 | 110 | [13] (S) | |||
Oct | ι Oct | V | 5,9 | 6,9 | 0,7″ | 2019 | RST 2819 | 12550-8507 | 110 | |||||||
Oct | λ Oct | V | 5,6 | 7,3 | 3,5″ | 2008 | HJ 5278 | 21509-8243 | 130 | |||||||
Oct | μ2 Oct | V | 6,5 | 7,1 | 16,6″ | 2015 | DUN 232 | 20417-7521 | 40 | |||||||
Oct | ν Oct | SB | 3,7 | . | – | – | 2,8 a | BLM 6 | 21415-7723 | 19 | ||||||
Oph | α Oph (Ras Alhague) | SI | 2,1 | 5,0 | 0,7″ | 2018 | 8,6 a | A5 IV | K5–7 V | 2,4 | 0,9 | MCY 4 | 17349+1234 | 15 | [160] (S, M) | |
Oph | η Oph | V | 3,1 | 3,3 | 0,5″ | 2019 | 88 a | A1 IV | A1 IV | 3,0 | 3,5 | BU 1118 | 17104-1544 | 27 | [60] (S), [161] (M) | |
Oph | λ Oph | 1 (AB/C) | CPM | 3,8 | 11,8 | 119,6″ | 2013 | A0 V + A4 V | Σ 4,8 | STF 2055 | 16309+0159 | 53 | [24] (S), [11] (M) | |||
2 (A/B) | V | 4,2 | 5,2 | 1,4″ | 2019 | 129 a | A0 V | A4 V | 2,7 | 2,1 | STF 2055 | |||||
Oph | ξ Oph | V | 4,4 | 8,9 | 4,1″ | 2015 | 420 a | F3 V | K3: | DON 832 | 17210-2107 | 17 | ||||
Oph | ο Oph | V | 5,2 | 6,6 | 10,8″ | 2019 | G8 III | F6 IV–V | H 3 25 | 17180-2417 | 86 | |||||
Oph | ρ Oph | V | 5,1 | 5,7 | 3,0″ | 2017 | 4200 a | B2 IV | B2 V | H 2 19 | 16256-2327 | 110 | ||||
Oph | τ Oph | 1 (A/B) | V | 5,3 | 5,9 | 1,5″ | 2019 | 260 a | F2 V | F5 V | STF 2262 | 18031-0811 | 51 | [3] (UAa/Ab), [13] (S) | ||
2 (Aa/Ab) | SB | 5,3 | . | – | – | 184 d | F2 V | |||||||||
Oph | υ Oph | 1 (A/B) | V | 4,7 | 8,8 | 1,0″ | 2019 | 76 a | A3m | Σ 5,0 ± 0,8 | RST 3949 | 16278-0822 | 41 | [3] (UAa/Ab), [58] (S, M) | ||
2 (Aa/Ab) | SB | 4,7 | . | – | – | 27,2 d | A3m | |||||||||
Oph | 19 Oph | O | 6,1 | 9,7 | 23,9″ | 2019 | STF 2096 | 16472+0204 | 220 | |||||||
Oph | 21 Oph | V | 5,8 | 7,3 | 0,8″ | 2019 | 990 a | STT 315 | 16514+0113 | 120 | ||||||
Oph | 24 Oph | V | 6,3 | 6,3 | 1,0″ | 2015 | 1100 a | BU 1117 | 16568-2309 | 120 | ||||||
Oph | 36 Oph | 1 (AB/C) | CPM | 4,4 | 6,5 | 731,6″ | 2000 | K0 V + K1 V | K5 V | Σ 1,6 | SHJ 243 | 17153-2636 | 5,9 | [162] (S, M) | ||
2 (A/B) | V | 5,1 | 5,1 | 5,1″ | 2017 | 470 a | K0 V | K1 V | 0,8 | 0,8 | SHJ 243 | |||||
Oph | 41 Oph | V | 4,9 | 7,5 | 0,7″ | 2019 | 141 a | A 2984 | 17166-0027 | 62 | ||||||
Oph | 47 Oph | I/SB | 4,9 | 5,8 | – | – | 26,3 d | 1,5 | 1,2 | MKT 14 | 17266-0505 | 31 | [163] (S, M, d) | |||
Oph | 61 Oph | V | 6,1 | 6,5 | 20,8″ | 2019 | A0 IV | A0 IV | STF 2202 | 17446+0235 | 97 | |||||
Oph | 68 Oph | V | 4,5 | 7,5 | 0,4″ | 2018 | 210 a | BU 1125 | 18018+0118 | 90 | ||||||
Oph | 70 Oph | V/SB | 4,2 | 6,2 | 6,4″ | 2019 | 88 a | K0 V | K5 V | 0,9 | 0,7 | STF 2272 | 18055+0230 | 5,1 | [49] (S, M) | |
Oph | 73 Oph | V | 6,0 | 7,5 | 0,8″ | 2019 | 290 a | A8 | F6 | 1,7 | 1,2 | STF 2281 | 18096+0400 | 55 | [11] (S, M) | |
Oph | HR 6367 | V | 6,3 | 7,8 | 0,7″ | 2018 | 200 a | A1 V | F3 V | A 1145 | 17082-0105 | 81 | [24] (S) | |||
Oph | HR 6516 | V | 6,1 | 6,2 | 0,4″ | 2019 | 46,4 a | G9 IV–V | G9 IV–V | 1,0 | 0,9 | STF 2173 | 17304-0104 | 16 | [1] (S, M, d) | |
Oph | V1054 Oph | 1 (ABC/F) | CPM | 9,0 | 16,9 | 230,7″ | 2005 | M3,5 Ve + M + M + M3,5 V | M7 Ve | Σ 1,2 | 0,08 | WNO 55 | 16555-0820 | 6,2 | [164] (UBa/Bb, SBa/Bb, M) | |
2 (AB/C) | CPM | 9,4 | 11,8 | 72,2″ | 2014 | M3,5 Ve + M + M | M3,5 V | Σ 1,0 | 0,2 | LDS 573 | ||||||
3 (A/B) | V/SB | 9,7 | 9,8 | 0,2″ | 2019 | 1,7 a | M3,5 Ve | M + M | 0,4 | Σ 0,6 | KUI 75 | |||||
4 (Ba/Bb) | SB | 9,8 | . | – | – | 2,97 d | M | M | 0,3 | 0,3 | ||||||
Oph | RS Oph | SB | 10,8 | . | – | – | 1,2 a | M0–2 III | D | 0,7–0,8 | 1,2–1,4 | 2400 | [30] (V), [165] (U, S, M) | |||
Ori | β Ori (Rigel) | 1 (A/BC) | V | 0,3 | 6,8 | 10,3″ | 2020 | B8 Iae | B9 + B9 | STF 668 | 05145-0812 | 260 | [3] (U) | |||
2 (B/C) | V | 7,5 | 7,6 | 0,1″ | 2005 | B9 | B9 | BU 555 | ||||||||
3 (Ba/Bb) | SB | 7,5 | . | – | – | 9,86 d | B9 | |||||||||
Ori | δ Ori (Mintaka) | 1 (Aa/Ab) | V | 2,4 | 3,8 | 0,3″ | 2019 | 350 a | O9,5 II + B0 V | B0 IV | Σ 32,3 | 22,5 | HEI 42 | 05320-0018 | 380 | [5] (UAa1/Aa2, SAa1/Aa2, MAa1/Aa2), [166] (SAb, MAb, d) |
2 (Aa1/Aa2) | E/SB | 2,5 | 5,6 | – | – | 5,73 d | O9,5 II | B0 V | 23,2 | 9,1 | ||||||
Ori | ζ Ori (Alnitak) | 1 (A/B) | V | 1,9 | 3,7 | 2,4″ | 2017 | 1510 a | O9,5 Ib + B0,5 IV | B0 III | Σ 47 ± 13 | STF 774 | 05407-0157 | 390 | [167] (S, M, d) | |
2 (Aa/Ab) | I/SB | 2,0 | 4,0 | – | – | 7,4 a | O9,5 Ib | B0,5 IV | 33 ± 10 | 14 ± 3 | NOI 1 | |||||
Ori | η Ori | 1 (A/B) | V | 3,6 | 4,9 | 1,9″ | 2020 | B1 V + B3 V + B2 V | B2: | DA 5 | 05245-0224 | 300 | [3] (UAa1/Aa2), [21] (SAa/Ab, SAa1/Ab2) | |||
2 (Aa/Ab) | SI/SB | 3,8 | 5,3 | 0,0″ | 2019 | 9,4 a | B1 V + B3 V | B2 V | MCA 18 | |||||||
3 (Aa1/Aa2) | E/SB | 3,8 | . | – | – | 7,98 d | B1 V | B3 V | ||||||||
Ori | θ1 Ori A | 1 (Aa/Ab) | SI | 6,6 | 9,8 | 0,2″ | 2018 | ≈ 210 a | B0,5 | Σ ≈ 18,5 | 4 | PTR 1 | 05353-0523 | 410 | [168] (U, S, M), [169] (d) | |
2 (Aa1/Aa2) | E | 6,6 | . | – | – | 65,1 d | B0,5 | ≈ 16 | ≈ 2,5 | |||||||
Ori | θ1 Ori B | 1 (Ba,Bc,Be/ Bb,Bd) |
SI | 7,5 | 8,5 | 0,9″ | 2012 | ≈ 1920– 11 000 a |
B1 V + A + B: | Σ ≈ 15 | Σ 7 | SMN 5 | 05353-0523 | 410 | [168] (U, S, M), [169] (d) | |
1? (Ba,Be/Bc) | SI | 7,5 | 10,5 | 0,6″ | 2012 | 2000 a | B1 V + A + B: | Σ ≈ 14 | ≈ 1 | SMN 5 | ||||||
2? (Bb/Bd) | SI | > 10 | > 10,8 | 0,1″ | 2012 | ≈ 200 a | 4 | 3 | PTR 1 | |||||||
3? (Ba/Be) | I | 7,5 | > 7,3 | – | – | B1 V + A | B: | Σ ≈ 9 | 4–6 | GVT 1 | ||||||
4? (Ba1/Ba2) | E | 7,5 | . | – | – | 6,47 d | B1 V | A | ≈ 7 | ≈ 2 | ||||||
Ori | θ1 Ori C | 1 (Ca/Cb) | I/SB | 5,3 | 6,7 | – | – | 11,4 a | O6 Vp | B0 V | Σ 33 ± 5 | 11 ± 5 | WGT 1 | 05353-0523 | 410 | [170] (SCa/Cb, MCa/Cb), [168] (UCa1/Ca2, MCa1/Ca2), [169] (d) |
2 (Ca1/Ca2) | SB | 5,3 | . | – | – | 61,5 d | O6 Vp | 31 | 1 | |||||||
Ori | θ1 Ori D | I/SB | 6,4 | > 6,9 | – | – | 53,0 d | B1,5 V | B | 16 | 6 | GVT 1 | 05353-0523 | 410 | [168] (U, S, M), [169] (d) | |
Ori | ι Ori | 1 (A/B) | V | 2,8 | 7,7 | 12,5″ | 2018 | O9 III + B1 III–IV + B2: IV: | B2 V | Σ > 36 | STF 752 | 05354-0555 | 410 | [171] (U, SAa1/Aa2, MAa1/Aa2), [81] (SAa/Ab, SB, d) | ||
2 (Aa/Ab) | SI | 3,0 | 6,3 | 0,1″ | 2016 | O9 III + B1 III–IV | B2: IV: | Σ 36 | CHR 250 | |||||||
3 (Aa1/Aa2) | SB | 3,0 | . | – | – | 29,1 d | O9 III | B1 III–IV | 23 | 13 | ||||||
Ori | λ Ori | V | 3,5 | 5,5 | 4,3″ | 2019 | O8 IIIf | B0,5 V | STF 738 | 05351+0956 | 340 | |||||
Ori | μ Ori | 1 (A/B) | V | 4,3 | 6,3 | 0,0″ | 2020 | 18,6 a | A5 V + G5 V | F5 V: + F5 V: | Σ 3,0 | Σ 2,7 | A 2715 | 06024+0939 | 46 | [33][134] (S, M, d) |
2 (Aa/Ab) | SB/A | 4,4 | . | – | – | 4,45 d | A5 V | G5 V | 2,4 | 0,7 | ||||||
2 (Ba/Bb) | SB/A | 6,3 | . | – | – | 4,78 d | F5 V: | F5 V: | 1,4 | 1,4 | ||||||
Ori | ρ Ori | 1 (A/B) | V | 4,6 | 8,5 | 6,4″ | 2018 | STF 654 | 05133+0252 | 110 | ||||||
2 (Aa/Ab) | SB/A | 4,5 | . | – | – | 2,8 a | ||||||||||
Ori | σ Ori | 1 (A/B) | V | 4,1 | 5,3 | 0,3″ | 2015 | 160 a | O9 V | B0,5 V | Σ 30 | 11,5 ± 1,5 | BU 1032 | 05387-0236 | 390 | [24] (S), [172] (UAa/Ab, M) |
2 (Aa/Ab) | I/SB | 4,1 | . | – | – | 143 d | O9 V | 17 | 12,8 | NOI 6 | ||||||
Ori | χ1 Ori | SI/SB | 4,5 | 7,5 | 0,0″ | 2019 | 14,1 a | G0 V | 1,0 | 0,15 | KNG 1 | 05544+2017 | 8,7 | [173] (S, M) | ||
Ori | 14 Ori | V | 5,7 | 6,6 | 1,0″ | 2020 | 198 a | Am | Am | 1,8 | 1,5 | STT 98 | 05079+0830 | 62 | [13] (S), [107] (M) | |
Ori | 23 Ori | V | 5,0 | 6,8 | 32,0″ | 2019 | B2 IV–V | B8–9 | STF 696 | 05228+0333 | 370 | |||||
Ori | 32 Ori | V | 4,5 | 5,8 | 1,3″ | 2017 | 610 a | B5 IV | B7 V | 4,4 | 3,3 | STF 728 | 05308+0557 | 93 | [24] (S), [11] (M) | |
Ori | 33 Ori | V | 5,7 | 6,7 | 1,8″ | 2017 | STF 729 | 05312+0318 | 350 | |||||||
Ori | 42 Ori | 1 (A/B) | V | 4,6 | 7,5 | 1,2″ | 2020 | B1 V | DA 4 | 05354-0450 | 400 | [174] (S, d) | ||||
2 (Aa/Ab) | SI | 4,9 | 6,3 | 0,2″ | 2020 | |||||||||||
Ori | 52 Ori | V | 6,0 | 6,0 | 1,0″ | 2019 | 1260 a | A5 V | F0 | STF 795 | 05480+0627 | 140 | [13] (S) | |||
Ori | 64 Ori | 1 (A/B) | SI/SB | 5,1 | 6,1 | 0,1″ | 2019 | 13,2 a | B7–8 IV–V + B7–8 IV–V | B5–6 IV–V | Σ 8,2 ± 0,7 | 3,8 ± 0,3 | MCA 24 | 06035+1941 | 270 | [3] (UAa/Ab), [175] (S, M) |
2 (Aa/Ab) | SB | 5,1 | . | – | – | 14,6 d | B7–8 IV–V | B7–8 IV–V | 4,3 ± 0,4 | 3,9 ± 0,3 | ||||||
Ori | 75 Ori | SI | 6,1 | 6,1 | 0,1″ | 2018 | 9,2 a | FIN 331 | 06171+0957 | 78 | ||||||
Ori | V1031 Ori | 1 (A/B) | SI | 6,3 | 7,8 | 0,2″ | 2019 | 31 a | A8 III–IV + A5 IV–V | A6 IV–V | Σ 4,8 | ≈ 2,2 | MCA 22 | 05474-1032 | 460 | [21] (UAa/Ab, S), [176] (M) |
2 (Aa/Ab) | E/SB | 6,3 | . | – | – | 3,41 d | A8 III–IV | A5 IV–V | 2,5 | 2,3 | ||||||
Ori | HR 2174 | V | 5,7 | 6,7 | 29,1″ | 2019 | B9 V | A2 IV | STF 855 | 06090+0230 | 180 | |||||
Pav | ξ Pav | 1 (A/B) | V | 4,5 | 8,1 | 3,7″ | 2016 | GLE 2 | 18232-6130 | 140 | ||||||
2 (Aa/Ab) | SB/A | 4,5 | . | – | – | 6,1 a | ||||||||||
Pav | HR 7278 | V | 6,1 | 6,4 | 0,5″ | 2019 | 157 a | A5 V | A8 V | GLE 3 | 19172-6640 | 92 | [13] (S) | |||
Pav | SCR 1845-6357 | V(aO) | 17,4 | . | 1,2″ | 2006 | M8,5 | T6 | 0,04–0,05 | BIL 1 | 18451-6358 | 3,9 | [30] (V), [177] (S, M, d) | |||
Peg | η Peg (Matar) | SI/SB | 4,1 | 6,9 | 0,1″ | 2005 | 2,2 a | G2 II–III | A5 V | 3,2 ± 0,4 | 2,0 ± 0,2 | BLA 11 | 22430+3013 | 73 | [178] (S, M) | |
Peg | ι Peg | I/SB | 3,5 | 5,7 | – | – | 10,2 d | F5 V | G8 V | 1,3 | 0,8 | PTI 1 | 22070+2521 | 11,5 | [33] (S, M) | |
Peg | κ Peg | 1 (A/B) | V/SB | 4,9 | 5,0 | 0,2″ | 2011 | 11,6 a | F5 IV | F5 IV + G–K | 1,5 | Σ 2,5 | BU 989 | 21446+2539 | 34 | [179] (S, M) |
2 (Ba/Bb) | SB/A | 5,0 | . | – | – | 5,97 d | F5 IV | G–K | 1,7 | 0,8 | ||||||
Peg | ψ Peg | SI | 4,7 | . | 0,1″ | 1995 | 55 a | MCA 76 | 23578+2508 | 150 | ||||||
Peg | 1 Peg | 1 (A/B) | CPM | 4,2 | 9,3 | 36,6″ | 2020 | 17 500 a | K1 III | K0 V | STFB 11 | 21221+1948 | 48 | [3] (UBa/Bb) | ||
2 (Ba/Bb) | SB | 9,3 | . | – | – | 3,0 a | K0 V | |||||||||
Peg | 3 Peg | CPM | 6,2 | 7,5 | 38,7″ | 2020 | A2 V | F0 V | STFA 56 | 21377+0637 | 88 | |||||
Peg | 13 Peg | V | 5,7 | 6,9 | 0,2″ | 2014 | 26,3 a | F2 III–IV | 2,7 ± 0,3 | COU 14 | 21501+1717 | 33 | [9] (M) | |||
Peg | 33 Peg | V | 6,3 | 9,2 | 1,0″ | 2017 | 410 a | F7 IV | STF 2900 | 22237+2051 | 33 | |||||
Peg | 34 Peg | 1 (A/B) | V | 5,8 | 12,5 | 4,1″ | 2015 | 420 a | F7 V | K4 | BU 290 | 22266+0424 | 40 | [13] (S) | ||
2 (Aa/Ab) | SB/A | 5,8 | . | – | – | 2,4 a | F7 V | |||||||||
Peg | 37 Peg | 1 (A/B) | V | 5,8 | 7,3 | 0,2″ | 2020 | 124 a | F4 IV | F7 IV | 1,7 | Σ 2,3 | STF 2912 | 22300+0426 | 53 | [24] (S), [180] (U, M) |
2 (Ba/Bb) | SI/SB | 7,8 | 8,2 | 0,0″ | 2020 | 2,1 a | F4 IV | 1,2 | 1,1 | STF 2912 | ||||||
Peg | 52 Peg | V | 6,1 | 7,3 | 0,5″ | 2016 | 250 a | A8 V | F6 V | STT 483 | 22592+1144 | 94 | [24] (S) | |||
Peg | 57 Peg | - (A/B) | O? | 5,2 | 10,1 | 32,6″ | 2015 | M4S III + A6 V | Σ ≈ 4,9 | STF 2982 | 23095+0841 | 240 | [181] (U, SAb, M) | |||
1 (Aa/Ab) | SI/SB | 5,2 | 8,2 | 0,2″ | 2014 | 100–500 a | M4S III | A6 V | ≈ 3 | ≈ 1,9 | YSC 16 | 23095+0841 | 240 | |||
Peg | 64 Peg | V | 5,4 | 7,8 | 0,4″ | 2002 | BU 718 | 23219+3149 | 170 | |||||||
Peg | 72 Peg | V | 5,7 | 6,1 | 0,6″ | 2018 | 490 a | K3 III | K5 III | ≈ 2 | ≈ 2 | BU 720 | 23340+3120 | 170 | [24] (S), [36] (M) | |
Peg | 78 Peg | V | 5,1 | 8,1 | 0,8″ | 2016 | 640 a | AGC 14 | 23440+2922 | 69 | ||||||
Peg | 85 Peg | V | 5,8 | 8,9 | 0,4″ | 2015 | 26,3 a | G3 V | K6 V | 0,9 | 0,7 | BU 733 | 00022+2705 | 13 | [49] (S, M) | |
Peg | IK Peg | SB | 6,1 | 14,4 | – | – | 21,7 d | A8 V | DA1,5 | 1,5 | 1,2 | 47 | [46] (V, U, S, M) | |||
Peg | EQ Peg | V | 10,5 | 12,4 | 5,4″ | 2017 | 230 a | M4 | M5 | WIR 1 | 23317+1956 | 6,2 | ||||
Per | β Per (Algol) | 1 (Aa/Ab) | SI/SB | 2,1 | 4,6 | 0,1″ | 2010 | 1,9 a | B8 V + K2 IV | Am | Σ 3,9 | 1,8 | LAB 2 | 03082+4057 | 28 | [182] (S, M) |
2 (Aa1/Aa2) | E/I/SB | 2,1 | . | – | – | 2,87 d | B8 V | K2 IV | 3,2 | 0,7 | CSI 1 | |||||
Per | γ Per | E/SI/SB | 3,6 | 3,8 | 0,1″ | 2007 | 14,6 a | G8 IIIa | A2 IV | 2,5 | 1,4 | WRH 29 | 03048+5330 | 75 | [5] (S, M) | |
Per | ε Per | 1 (A/B) | V | 2,9 | 8,9 | 8,8″ | 2020 | B1,5 III | A2 V | Σ ≈ 15 | STF 471 | 03579+4001 | 200 | [183] (U, M) | ||
2 (Aa/Ab) | SB | 2,9 | . | – | – | 14,1 d | B1,5 III | 13,5 ± 2,0 | 0,9–1,8 | |||||||
Per | ζ Per | 1 (A/E) | CPM | 2,9 | 10,0 | 120,0″ | 2012 | B1 Ib + B9 V | A2V | STF 464 | 03541+3153 | 230 | ||||
2 (A/B) | V | 2,9 | 9,2 | 12,8″ | 2020 | B1 Ib | B9 V | STF 464 | ||||||||
Per | η Per (Miram) | CPM | 3,8 | 8,5 | 28,7″ | 2018 | K3 Ib–IIa | B9 V | STF 307 | 02507+5554 | 270 | |||||
Per | θ Per | V | 4,2 | 10,0 | 21,2″ | 2020 | 2700 a | F7 V | M1 V | STF 296 | 02442+4914 | 11,1 | [24] (S) | |||
Per | ο Per | 1 (A/B) | V | 3,9 | 6,7 | 1,1″ | 2015 | B1 III + B2 V | Σ 24 | BU 535 | 03443+3217 | 340 | [184] (U, S), [185] (M) | |||
2 (Aa/Ab) | SB | 3,9 | . | – | – | 4,42 d | B1 III | B2 V | 14 | 10 | ||||||
Per | τ Per | E/SI/SB | 4,2 | 5,9 | – | – | 4,1 a | G8 IIIa | A6 V | 2,1 | 1,8 | LAB 1 | 02543+5246 | 64 | [5] (S, M) | |
Per | φ Per | SI/SB | 4,1 | 7,8 | 0,0″ | 2013 | 127 d | Be | sdO | CIA 6 | 01437+5041 | 220 | [60] (S) | |||
Per | 12 Per | SI/SB | 5,5 | 5,9 | 0,0″ | 2016 | 331 d | F8 V | G1,5 V | 1,4 | 1,2 | MCA 8 | 02422+4012 | 24 | [33] (S, M, d) | |
Per | 20 Per | 1 (AB/C) | V | 5,4 | 9,7 | 14,0″ | 2014 | F3 IV–V + F6 IV–V | Σ 3,9 ± 0,6 | STF 318 | 02537+3820 | 71 | [24] (S), [9] (M) | |||
2 (A/B) | V | 5,8 | 6,8 | 0,2″ | 2008 | 31,6 a | F3 IV–V | F6 IV–V | Σ 3,9 ± 0,6 | BU 524 | ||||||
Per | 34 Per | V | 4,7 | 7,3 | 0,6″ | 2016 | BU 1179 | 03294+4931 | 170 | |||||||
Per | 56 Per | 1 (A/B) | V | 5,8 | 9,3 | 4,2″ | 2017 | 1890 a | F4 V + DA3,1 | F2 | Σ 2,4 | STT 81 | 04246+3358 | 41 | [46] (UAa/Ab, SAa/Ab, M) | |
2 (Aa/Ab) | V(HST) | 5,8 | 15,0 | 0,4″ | 1999 | 47 a | F4 V | DA3,1 | 1,5 | 0,9 | BAS 5 | |||||
2 (Ba/Bb) | V(HST) | 9,6 | 11,3 | 0,6″ | 2002 | F2 | BAS 5 | |||||||||
Per | 57 Per | O | 6,1 | 6,8 | 121,4″ | 2013 | F0 V | F0 | SHJ 44 | 04334+4304 | 61 | |||||
Per | 58 Per | SB/A | 4,3 | . | – | – | 28,8 a | K0 II–III | B9 V | 58 Per | 04367+4116 | 240 | ||||
Per | HR 890 | V | 5,2 | 6,2 | 12,0″ | 2019 | B7 V | B9 V | STF 331 | 03009+5221 | 140 | |||||
Phe | α Phe | SB/A | 2,4 | . | – | – | 10,5 a | alp Phe | 00262-4217 | 26 | ||||||
Phe | β Phe | V | 4,1 | 4,2 | 0,6″ | 2018 | 171 a | SLR 1 | 01061-4643 | 50 | [186] (d) | |||||
Phe | γ Phe | SB/A | 3,4 | . | – | – | 194 d | gam Phe | 01284-4319 | 72 | ||||||
Phe | ζ Phe | 1 (AB/C) | V | 4,0 | 8,2 | 6,8″ | 2016 | B6 V + B8 V + A7 V | F1 V | Σ 8,1 | RMK 2 | 01084-5515 | 92 | [21] (UAa/Ab, SB, MB), [33] (SAa/Ab, MAa/Ab) | ||
2 (A/B) | V | 4,0 | 6,8 | 0,6″ | 2020 | 290 a | B6 V | A7 V | Σ 6,4 | 1,7 | RST 1205 | |||||
3 (Aa/Ab) | E/SB | 4,0 | . | – | – | 1,67 d | B6 V | B8 V | 3,9 | 2,5 | ||||||
Phe | η Phe | 1 (A/B) | V | 4,4 | 11,5 | 20,1″ | 1999 | A0 IV + G:–K: | HJ 3391 | 00434-5728 | 76 | [136] (U, S, M) | ||||
2 (Aa/Ab) | I/A | 4,4 | 8,5 | – | – | ≈ 10 a | A0 IV | G:–K: | 2,8 | MRN 1 | ||||||
Phe | ξ Phe | V | 5,7 | 10,0 | 13,1″ | 2015 | HJ 3387 | 00418-5630 | 68 | |||||||
Phe | υ Phe | V | 5,5 | 6,9 | 0,3″ | 2020 | 28,4 a | A2 IV | A4 IV | Σ 3,2 ± 0,4 | RST 3352 | 01078-4129 | 62 | [13] (S), [58] (M) | ||
Pic | α Pic | A | 3,3 | . | – | – | 4,2 a | alp Pic | 06482-6156 | 30 | ||||||
Pic | θ Pic | 1 (AB/C) | CPM | 6,2 | 6,7 | 38,3″ | 2008 | A0 V | A2 V | DUN 20 | 05248-5219 | 160 | ||||
2 (A/B) | V | 6,8 | 7,4 | 0,3″ | 2019 | 123 a | A0 V | I 345 | ||||||||
Pic | ι Pic | V | 5,6 | 6,2 | 12,8″ | 2009 | DUN 18 | 04509-5328 | 40 | |||||||
Pic | μ Pic | V | 5,6 | 9,3 | 2,5″ | 2019 | B9I Vn | A8 V:p | HJ 3874 | 06320-5845 | 190 | |||||
PsA | α PsA (Fomalhaut) | 1 (AB/C) | CPM | 1,2 | 12,6 | 5,7° | – | A3 Va + K4e | M4 V | Σ 2,6 | 0,2 | MAM 1 | 22577-2937 | 7,7 | [187] (ρAB/C, ρA/B, S, M) | |
2 (A / B = TW PsA) | CPM | 1,2 | 6,6 | 2,0° | – | A3 Va | K4e | 1,9 | 0,7 | SHY 106 | ||||||
PsA | β PsA | V | 4,3 | 7,1 | 30,4″ | 2015 | A1 Va | G1 V | PZ 7 | 22315-3221 | 44 | |||||
PsA | γ PsA | V | 4,5 | 8,2 | 4,0″ | 2010 | A0 VpSrCrEu | F5 V | HJ 5367 | 22525-3253 | 62 | |||||
PsA | δ PsA | V | 4,3 | 9,2 | 4,9″ | 2015 | HWE 91 | 22559-3232 | 53 | |||||||
PsA | η PsA | V | 5,7 | 6,8 | 1,9″ | 2017 | B8(shell) III | B8,5 IV | BU 276 | 22008-2827 | 250 | |||||
PsA | θ PsA | SI | 5,8 | 5,8 | 0,1″ | 2020 | 20,0 a | A1 V | A1 V | 2,3 ± 0,4 | 2,3 ± 0,4 | FIN 330 | 21477-3054 | 90 | [16] (S, M, d) | |
Psc | α Psc (Alrescha) | V | 4,1 | 5,2 | 1,9″ | 2019 | 1950 a | kA0hA7Sr | kA2hF2mF2 | STF 202 | 02020+0246 | 46 | ||||
Psc | ζ Psc | 1 (A/BC) | V | 5,2 | 6,3 | 23,1″ | 2020 | A7 IV | F7 V + G7 V | STF 100 | 01137+0735 | 40 | [3] (U, SBa/Bb) | |||
2 (B/C) | V | 6,3 | 12,2 | 2,0″ | 2015 | F7 V + G7 V | BU 1029 | |||||||||
3 (Ba/Bb) | SB | 6,3 | . | – | – | 9,08 d | F7 V | G7 V | ||||||||
Psc | η Psc | V | 3,8 | 7,5 | 0,6″ | 2008 | 850 a | BU 506 | 01315+1521 | 110 | ||||||
Psc | ψ1 Psc | 1 (A/B) | V | 5,3 | 5,5 | 29,9″ | 2020 | A0 IV–Vnn | B9 IVn | STF 88 | 01057+2128 | 84 | ||||
2 (Aa/Ab) | SI | 5,7 | 6,6 | 0,1″ | 2017 | 14,4 a | A0 IV–Vnn | YR 6 | ||||||||
Psc | 24 Psc | SI | 6,7 | 6,7 | 0,1″ | 2020 | 22,8 a | G9 III | A0 V | Σ 2,9 ± 0,8 | FIN 359 | 23529-0309 | 170 | [20] (S, M) | ||
Psc | 27 Psc | V | 4,9 | 8,9 | 0,7″ | 2018 | 930 a | BU 730 | 23587-0333 | 72 | ||||||
Psc | 33 Psc | SB/A | 4,6 | . | – | – | 72,9 d | 1,7 ± 0,4 | 0,8 ± 0,2 | 33 Psc | 00053-0542 | 39 | [188] (M) | |||
Psc | 34 Psc | V | 5,5 | 9,4 | 7,6″ | 2015 | B9 Vn | G5 Ve | STF 5 | 00100+1109 | 93 | |||||
Psc | 35 Psc | 1 (A/B) | V | 6,1 | 7,5 | 11,2″ | 2019 | F1 IV–V + F1 IV–V | A7 | STF 12 | 00150+0849 | 75 | [3] (U, SAa/Ab) | |||
2 (Aa/Ab) | E/SB | 6,1 | . | – | – | 0,84 d | F1 IV–V | F1 IV–V | ||||||||
Psc | 51 Psc | SI | 5,8 | 8,0 | 0,2″ | 2020 | 27,5 a | MCA 1 | 00324+0657 | 89 | ||||||
Psc | 55 Psc | V | 5,6 | 8,5 | 6,6″ | 2015 | K2 IIIa | F3 V | STF 46 | 00399+2126 | 130 | |||||
Psc | 64 Psc | SB | 5,7 | 6,0 | – | – | 13,8 d | F8 V | F8 V | 1,2 | 1,2 | 64 Psc | 00490+1656 | 23 | [18] (V), [33] (S, M, d) | |
Psc | 65 Psc | V | 6,3 | 6,3 | 4,4″ | 2020 | F5 III | F4 III | STF 61 | 00499+2743 | 89 | |||||
Psc | 66 Psc | V | 6,1 | 7,2 | 0,6″ | 2018 | 340 a | A0 V | A4 V | STT 20 | 00546+1911 | 77 | [24] (S) | |||
Psc | 77 Psc | 1 (A/B) | V | 6,4 | 7,3 | 33,2″ | 2020 | F5 V | F5–7 V | STF 90 | 01058+0455 | 45 | ||||
Psc | 103 Psc | V | 7,0 | 9,2 | 0,6″ | 2008 | BU 5 | 01393+1638 | 180 | |||||||
Pup | π Pup | 1 (A/B) | CPM | 2,9 | 7,9 | 66,5″ | 2009 | K4 III + B5 | B9–A0 V | DUN 43 | 07171-3706 | 250 | ||||
2 (Aa/Ab) | 2,9 | 6,5 | 0,7″ | 1991 | K4 III | B5 | HDS 1008 | |||||||||
Pup | σ Pup | 1 (A/B) | V | 3,3 | 8,8 | 22,1″ | 2015 | K5 III + A: | G5 V | Σ ≈ 7 | DUN 51 | 07292-4318 | 59 | [189] (S, M) | ||
2 (Aa/Ab) | SB/A | 3,3 | . | – | – | 258 d | K5 III | A: | ≈ 5 | ≈ 2 | sig Pup | |||||
Pup | d2 Pup | V | 5,8 | 8,6 | 1,2″ | 1996 | I 160 | 07397-3808 | 180 | |||||||
Pup | f Pup | SI | 4,8 | 6,1 | 0,1″ | 2020 | 81 a | FIN 324 | 07374-3458 | 110 | ||||||
Pup | G Pup | V | 5,9 | 8,1 | 1,0″ | 1999 | I 156 | 06257-4811 | 180 | |||||||
Pup | k Pup (HR 2949 / 2948) | O | 4,4 | 4,6 | 9,9″ | 2016 | B5 IV | B6 V | H 3 27 | 07388-2648 | 120 | |||||
Pup | n Pup | V | 5,8 | 5,9 | 9,9″ | 2015 | F5 V | F6 V | H N 19 | 07343-2328 | 32 | |||||
Pup | t Pup | SI | 5,1 | 7,6 | 0,0″ | 2020 | 52 a | HDS 970 | 06584-3407 | 170 | ||||||
Pup | 2 Pup | 1 (A/B) | V | 6,0 | 6,7 | 16,7″ | 2019 | A2 V | A8 V + A8 V | ≈ 2 | Σ 3,2 | STF 1138 | 07455-1441 | 86 | [21] (U, S), [190] (M) | |
2 (Ba/Bb) | E/SB | 6,7 | . | – | – | 1,66 d | A8 V | A8 V | 1,6 | 1,6 | ||||||
Pup | 5 Pup | V | 5,7 | 7,3 | 1,0″ | 2020 | 570 a | F5 | G3 | STF 1146 | 07479-1212 | 29 | [13] (S) | |||
Pup | 9 Pup | V/SB | 5,6 | 6,5 | 0,4″ | 2019 | 23,3 a | F9 V | G4 V | 1,2 | 0,9 | BU 101 | 07518-1354 | 17 | [13] (S), [68] (M) | |
Pup | 171 G. Pup | 1 (A/B) | CPM | 5,3 | 14,7 | 871,1″ | 2010 | F9 V | DC10 | RAG 6 | 07456-3410 | 15 | ||||
2 (Aa/Ab) | SI | 5,3 | 9,0 | 0,8″ | 2020 | 23,1 a | F9 V | TOK 193 | ||||||||
Pup | 188 G. Pup | SI | 5,6 | 6,8 | 0,0″ | 2020 | 2,4 a | G1,5 IIIFe | A: | Σ ≈ 5,9 | TOK 194 | 07490-2455 | 110 | [191] (SB, M) | ||
Pup | HR 2668 | 1 (AB/C) | CPM | 5,3 | 8,8 | 185,0″ | 2015 | K0,5 V + G1,5 V | K6 V | DUN 38 | 07040-4337 | 17 | ||||
2 (A/B) | V | 5,6 | 6,7 | 21,2″ | 2015 | K0,5 V | G1,5 V | DUN 38 | ||||||||
2 (Ca/Cb) | SI/SB | 8,8 | 13,0 | 0,2″ | 2020 | 4,6 a | K6 V | TOK 390 | ||||||||
Pup | HR 3143 | CPM | 6,2 | 6,2 | 16,3″ | 2010 | B2–3 | B2–3 | DUN 59 | 07592-4959 | 430 | |||||
Pyx | ε Pyx | 1 (A/BC) | V | 5,6 | 9,5 | 17,6″ | 2015 | H N 96 | 09099-3022 | 65 | ||||||
2 (B/C) | V | 10,5 | 10,8 | 0,2″ | 2020 | B 1113 | ||||||||||
Pyx | XY Pyx | 1 (Aa/Ab) | SI | 6,1 | 7,0 | 0,1″ | 2018 | 66 a | B2 V | FIN 314 | 08280-3507 | 620 | [60] (UAa1/Aa2) | |||
2 (Aa1/Aa2) | E | 6,1 | . | – | – | 0,92 d | B2 V | |||||||||
Pyx | HR 3367 | V | 5,8 | 6,7 | 0,4″ | 2019 | 260 a | I 489 | 08315-1935 | 110 | ||||||
Pyx | HR 3430 | V | 5,4 | 6,8 | 0,7″ | 2018 | 123 a | G3 V | K0 V | BU 208 | 08391-2240 | 19 | [24] (S) | |||
Ret | β Ret | SI/SB | 4,0 | 6,8 | 0,1″ | 2019 | 5,2 a | TOK 191 | 03442-6448 | 31 | ||||||
Ret | ε Ret | V | 4,4 | 12,5 | 13,0″ | 2015 | K2 IV | DA3,3 | JSP 56 | 04165-5918 | 18 | [46] (S) | ||||
Ret | ζ Ret | CPM | 5,3 | 5,6 | 309,1″ | 2015 | G2,5 V | G1 V | 1,0 | 1,0 | ALB 1 | 03182-6230 | 12 | [192] (M) | ||
Ret | θ Ret | V | 6,0 | 7,7 | 4,1″ | 2015 | 26 000 a | B9 IV | kA2hA5VmA7 | RMK 3 | 04177-6315 | 140 | ||||
Scl | ε Scl | V | 5,4 | 8,5 | 5,0″ | 2017 | 2200 a | F0 V | G9 V | HJ 3461 | 01456-2503 | 28 | [24] (S) | |||
Scl | κ1 Scl | V | 6,1 | 6,2 | 1,3″ | 2017 | 580 a | F4 III | F3 III | BU 391 | 00094-2759 | 77 | [13] (S) | |||
Scl | λ1 Scl | V | 6,6 | 7,0 | 0,7″ | 2017 | HDO 182 | 00427-3828 | 150 | |||||||
Scl | τ Scl | V | 6,0 | 7,4 | 0,8″ | 2020 | 680 a | 1,9 | 1,4 | HJ 3447 | 01361-2954 | 54 | [11] (M) | |||
Sco | α Sco (Antares) | V | 1,0 | 5,4 | 2,8″ | 2019 | 2700 a | M0,5 Iab | B3 V: | 12 | 7 | GNT 1 | 16294-2626 | 170 | [193] (M1), [194] (M2) | |
Sco | β Sco (Akrab) | 1 (β1 = AB / β2 = CE) | V | 2,6 | 4,5 | 13,4″ | 2019 | B1 V | B2 V + B8pMn | Σ 33 | H 3 7 | 16054-1948 | 140 | [195] (UEa/Eb, SEa), [196] (MAa/Ab, MC, MEa, SAa/Ab), [197] (MB) | ||
2 (A/B) | V | 2,6 | 10,6 | 0,3″ | 2019 | 640 a | B1 V | Σ 25 | 8 | BU 947 | ||||||
2 (C/E) | SI | 4,5 | 6,6 | 0,1″ | 2019 | 19 a | B2 V | B8pMn | 8 | MCA 42 | ||||||
3 (Aa/Ab) | SB | 2,9 | 4,1 | – | – | 6,83 d | B0,5 IV–V | B1,5 V | 15 | 10 | OCC 1958 | |||||
3 (Ea/Eb) | SB | 6,6 | . | – | – | 11,1 d | B8pMn | 3,5 | ||||||||
Sco | δ Sco | SI/SB | 2,4 | 4,6 | 0,2″ | 2019 | 10,8 a | B0,3 IV | 13 | 8,2 | LAB 3 | 16003-2237 | 150 | [198] (S, M) | ||
Sco | λ Sco | 1 (A/B) | I/SB | 2,1 | 2,7 | – | – | 2,9 a | B1,5 IV | B2 IV | Σ 12,2 ± 1,5 | 8,1 ± 1,0 | TNG 1 | 17336-3706 | 110 | [199] (UAa/Ab, S, M, d) |
2 (Aa/Ab) | SB | 2,1 | . | – | – | 6 d | B1,5 IV | 10,4 ± 1,3 | 1,8 ± 0,2 | |||||||
Sco | θ Sco | V | 2,0 | 5,4 | 6,5″ | 1991 | SEE 510 | 17373-4300 | 92 | |||||||
Sco | ν Sco | 1 (AB/CD) | CPM | 4,0 | 6,1 | 41,3″ | 2019 | B2 V | B8 V + B9 VpSi | Σ 23 | Σ 8,4 | H 5 6 | 16120-1928 | 150 | [3] (UAa/Ab), [13] (SC/D), [200] (M) | |
2 (A/B) | V | 4,4 | 5,3 | 1,3″ | 2019 | B2 V | Σ 17 | 6 | BU 120 | |||||||
2 (C/D) | V | 6,6 | 7,2 | 2,4″ | 2019 | B8 V | B9 VpSi | 3 | Σ 5,4 | MTL 2 | ||||||
3 (Aa,Ab/Ac) | SI | 4,5 | 6,8 | 0,1″ | 2019 | B2 V | Σ 11 | 6 | CHR 146 | |||||||
4 (Aa/Ab) | SB | 4,5 | . | – | – | 5,6 d | B2 V | 10 | ≈ 1 | |||||||
Sco | ξ Sco | 1 (ABC/DE) | CPM | 4,1 | 7,4 | 282,0″ | – | ≈ 300 000 a | F5 IV + F5 IV + G1 V | G8 V + K0 V | Σ 4,0 | Σ 1,9 | 23 | [24] (SA/B), [201] (ρABC/DE, UABC/DE, UAB/C, UD/E, SC, SD/E, M) | ||
2 (AB/C) | V | 4,2 | 7,3 | 7,2″ | 2019 | 1510 a | F5 IV + F5 IV | G1 V | Σ 3,0 | 1,0 | STF 1998 | 16044-1122 | ||||
2 (D/E) | V | 7,4 | 8,0 | 11,9″ | 2019 | ≈ 4500 a | G8 V | K0 V | 1,0 | 0,9 | STF 1999 | 16044-1127 | ||||
3 (A/B) | V | 4,8 | 4,9 | 1,2″ | 2020 | 45,9 a | F5 IV | F5 IV | 1,5 | 1,5 | STF 1998 | 16044-1122 | ||||
Sco | π Sco | E/SB | 2,9 | . | – | – | 1,57 d | B1 V | B2: V: | 15589-2607 | 180 | [3] (U) | ||||
Sco | ρ Sco | SB | 3,9 | . | – | – | 4,00 d | B2 IV–V | 15569-2913 | 140 | [3] (U, S) | |||||
Sco | σ Sco | 1 (A/B) | CPM | 2,9 | 8,4 | 20,5″ | 2019 | B1 III + B1 V + B7 V | B9,5 V | H 4 121 | 16212-2536 | 210 | [202] (S, M) | |||
2 (Aa/Ab) | SI | 3,1 | 5,2 | 0,4″ | 2019 | B1 III + B1 V | B7 V | Σ 22,2 +1,6−2,6 | BLM 4 | |||||||
3 (Aa1/Aa2) | I/SB | 3,3 | 4,1 | – | – | 33,0 d | B1 III | B1 V | 13,5 +0,5−1,4 | 8,7 +0,6−1,2 | NOR 1 | |||||
Sco | 2 Sco | V | 4,7 | 7,0 | 2,0″ | 2019 | BU 36 | 15536-2520 | 150 | |||||||
Sco | 11 Sco | V | 5,8 | 9,8 | 3,3″ | 2015 | BU 39 | 16076-1245 | 120 | |||||||
Sco | 12 Sco | V | 5,8 | 8,1 | 3,8″ | 2016 | B9 V | F3 V | HJ 4839 | 16123-2825 | 93 | |||||
Sco | HR 6077 | V | 5,6 | 6,9 | 23,6″ | 2018 | F5 IV | F9 V | BSO 12 | 16195-3054 | 44 | |||||
Sco | Gliese 667 | 1 (AB/C) | V | 6,0 | 10,3 | 32,7″ | 2019 | K3 V + K5 V | M1,5 V | HJ 4935 | 17190-3459 | 6,8 | ||||
2 (A/B) | V | 6,4 | 7,4 | 0,7″ | 2019 | 42,2 a | K3 V | K5 V | MLO 4 | |||||||
Sct | β Sct | I/SB | 4,3 | 8,1 | – | – | 2,3 a | G4 IIa | B9 V | 4,6 | 2,6 | NOI 5 | 18472-0445 | 220 | [203] (V), [204] (S, M) | |
Ser | β Ser | V | 3,7 | 10,0 | 29,4″ | 2019 | A2 IV | K3 V | STF 1970 | 15462+1525 | 48 | |||||
Ser | δ Ser | V | 4,2 | 5,2 | 4,0″ | 2020 | 1150 a | F0 IV | F0 IV | STF 1954 | 15348+1032 | 70 | ||||
Ser | θ Ser | V | 4,6 | 4,9 | 22,4″ | 2019 | A5 V | A5 Vn | STF 2417 | 18562+0412 | 40 | |||||
Ser | ι Ser | V | 5,4 | 5,2 | 0,2″ | 2012 | 21,9 a | B9 V | A1 V | 2,0 ± 0,4 | 2,0 ± 0,4 | HU 580 | 15416+1940 | 58 | [112] (S, M) | |
Ser | μ Ser | SI | 3,8 | 5,4 | 0,4″ | 2018 | 71 a | CHR 259 | 15496-0326 | 52 | ||||||
Ser | ψ Ser | 1 (A/B) | V | 6,0 | 12,0 | 4,6″ | 2013 | 730 a | G3 V | M3 + M3 | A 2230 | 15440+0231 | 15 | [60] (S) | ||
2 (Ba/Bb) | V(aO) | 12,7 | 12,8 | 0,1″ | 2020 | M3 | M3 | RDR 6 | ||||||||
Ser | 36 Ser | SI | 5,2 | 7,8 | 0,4″ | 2018 | 65 a | A7 | G0 | Σ 3,1 ± 0,5 | CHR 51 | 15513-0305 | 50 | [20] (S, M) | ||
Ser | 59 Ser | V | 5,4 | 7,6 | 3,9″ | 2018 | A0 Vs | G: III | STF 2316 | 18272+0012 | 140 | |||||
Ser | HR 7048 („Tweedledum and Tweedledee“) | 1 (A/B) | V | 6,3 | 6,7 | 2,6″ | 2019 | A1 V + A | A2 V + A | Σ 10–12 | STF 2375 | 18455+0530 | 190 | [205] (SAb, SBb, M) | ||
2 (Aa/Ab) | SI | 6,9 | 7,3 | 0,0″ | 2020 | 28 a | A1 V | A | Σ 5–6 | FIN 332 | ||||||
2 (Ba/Bb) | SI | 7,5 | 7,5 | 0,1″ | 2020 | 40 a | A2 V | A | Σ 5–6 | FIN 332 | ||||||
Sex | γ Sex | V | 5,4 | 6,4 | 0,5″ | 2019 | 78 a | A1 V | A4 V | AC 5 | 09525-0806 | 85 | [24] (S) | |||
Sex | 35 Sex | V | 6,2 | 7,1 | 6,8″ | 2019 | K2 II–III | K1 II–III | STF 1466 | 10433+0445 | 170 | |||||
Sex | 40 Sex | V | 7,1 | 7,8 | 2,4″ | 2017 | STF 1476 | 10493-0401 | 86 | |||||||
Sge | δ Sge | SI/SB | 4,3 | 5,0 | 0,1″ | 1991 | 10,1 a | M2 IIab | B9,5 V | 3,9 | 3,5 | BLA 6 | 19474+1832 | 130 | [5] (S, M) | |
Sge | ζ Sge | 1 (AB/C) | V | 5,0 | 9,0 | 8,3″ | 2016 | A1 V + A3 V | F5 | Σ 4,7 ± 1,2 | STF 2585 | 19490+1909 | 78 | [206] (S), [9] (M) | ||
2 (A/B) | V | 5,6 | 6,0 | 0,2″ | 2007 | 23,2 a | A1 V | A3 V | Σ 4,7 ± 1,2 | AGC 11 | ||||||
Sge | θ Sge | - (AB/C) | O | 6,4 | 7,5 | 91,3″ | 2017 | F3 V + G5 V | K2 III | STF 2637 | 20099+2055 | 45 | ||||
1 (A/B) | V | 6,6 | 8,9 | 11,7″ | 2019 | F3 V | G5 V | STF 2637 | 20099+2055 | 260 | ||||||
Sgr | β1 Sgr | O? | 4,0 | 7,2 | 28,4″ | 2010 | B9 V | F0 V | DUN 226 | 19226-4428 | 80 | |||||
Sgr | ζ Sgr | V | 3,3 | 3,5 | 0,3″ | 2020 | 21,0 a | A2 III | A4 IV | Σ 5,3 ± 0,4 | HDO 150 | 19026-2953 | 27 | [13] (S), [58] (M) | ||
Sgr | η Sgr | V | 3,3 | 8,0 | 3,5″ | 2016 | BU 760 | 18176-3646 | 45 | |||||||
Sgr | κ2 Sgr | V | 5,7 | 7,3 | 0,4″ | 2017 | 700 a | BU 763 | 20239-4225 | 96 | ||||||
Sgr | τ Sgr | A | 3,3 | . | – | – | 69,3 d | tau Sgr | 19069-2740 | 36 | ||||||
Sgr | υ Sgr | SB/A | 4,6 | . | – | – | 138 d | B8p | F2pe | ups Sgr | 19217-1557 | 550 | [3] (S) | |||
Sgr | χ1 Sgr | SI | 5,8 | 5,8 | 0,1″ | 2020 | 5,7 a | A8 | A6–F0 | FIN 327 | 19253-2431 | 77 | [13] (S) | |||
Sgr | ψ Sgr | 1 (A/B) | V | 5,5 | 5,7 | 0,1″ | 2019 | 20,0 a | K2 III | A9 III + A3 V | 3,1 ± 0,6 | Σ 4,4 ± 0,7 | B 430 | 19155-2515 | 91 | [3] (UBa/Bb), [2] (S, M) |
2 (Ba/Bb) | SB | 5,7 | . | – | – | 10,8 d | A9 III | A3 V | 2,4 ± 0,1 | 2,0 ± 0,6 | ||||||
Sgr | 17 Sgr | SI | 7,2 | 8,9 | 0,1″ | 2020 | 119 a | MCA 51 | 18166-2033 | 210 | ||||||
Sgr | 21 Sgr | V | 5,0 | 7,4 | 1,7″ | 2008 | JC 6 | 18254-2033 | 140 | |||||||
Sgr | 52 Sgr | V | 4,7 | 9,2 | 2,4″ | 1999 | BU 654 | 19367-2453 | 58 | |||||||
Sgr | W Sgr | 1 (Aa/Ab) | SI | 4,7 | . | 0,2″ | 2002 | ≈ 173 a | G0 Ib–II + F5 | A0 V | Σ ≈ 7 | ≈ 2,2 | BLM 5 | 18050-2935 | 850 | [19][207] (U, SAa1/Aa2, SAb, M) |
2 (Aa1/Aa2) | SB/A | 4,7 | . | – | – | 4,3 a | G0 Ib–II | F5 | ≈ 5,8 | ≤ 1,4 | W Sgr | |||||
Sgr | Gliese 783 | V | 5,3 | 11,5 | 4,3″ | 2013 | K2,5 V | M3,5 | HJ 5173 | 20112-3606 | 6,0 | |||||
Sgr | WR 104 | 1 (WR,OB/B) | V(HST) | 13,6 | 15,4 | 1,0″ | 1998 | ≈ 47 a | WC9 + B0,5 V | O8–5 V | Σ 30 | 2600 | [208] (V, ρ, Ep.), [209] (U, S, M, d) | |||
2 (WR/OB) | 13,6 | . | – | – | 242 d | WC9 | B0,5 V | 10 | 20 | |||||||
Tau | δ3 Tau | V | 4,3 | 7,9 | 1,8″ | 2010 | KUI 17 | 04255+1756 | 46 | |||||||
Tau | θ Tau | 1 (θ2 = A / θ1 = B) | CPM | 3,4 | 3,8 | 347,9″ | 2016 | K0 IIIb | A7 III | 5,1 | Σ 4,2 ± 1,1 | STFA 10 | 04287+1552 | 48 | [210] (SAa/Ab, MAa/Ab), [211] (SBa/Bb, MBa/Bb, d) | |
2 (Aa/Ab) | I/SB | 3,7 | 4,9 | – | – | 141 d | A7 III | 2,9 | 2,2 | MKT 13 | ||||||
2 (Ba/Bb) | SI/SB | 3,8 | 7,3 | 0,2″ | 2020 | 16,3 a | K0 IIIb | 2,9 ± 0,9 | 1,3 ± 0,2 | MCA 15 | ||||||
Tau | κ Tau | CPM | 4,2 | 5,3 | 339,4″ | 2016 | A7 IV–V | F0 Vn | STF 541 | 04254+2218 | 47 | |||||
Tau | ξ Tau | 1 (A/B) | SI | 3,7 | 7,6 | 0,6″ | 2020 | 51 a | B9 V + B9 V + B5 V | F5 V | Σ 8,3 | 0,9 | HDS 433 | 03272+0944 | 61 | [212] (S, M) |
2 (Aa/Ab) | I/SB | 4,8 | 4,3 | – | – | 145 d | B9 V + B9 V | B5 V | Σ 4,4 | 3,9 | MKT 15 | |||||
3 (Aa1/Aa2) | E/SB | 4,8 | . | – | – | 7,15 d | B9 V | B9 V | 2,3 | 2,1 | ||||||
Tau | σ Tau | CPM | 4,7 | 5,1 | 444,0″ | 2014 | STFA 11 | 04393+1555 | 48 | |||||||
Tau | τ Tau | 1 (A/B) | CPM | 4,2 | 7,0 | 62,5″ | 2017 | B3 V | A2 | S 455 | 04422+2257 | 93 | ||||
2 (Aa/Ab) | SI | 4,3 | 7,0 | 0,3″ | 2007 | 58 a | B3 V | MCA 16 | ||||||||
Tau | χ Tau | 1 (A/B) | V | 5,4 | 8,5 | 19,4″ | 2016 | B9 V | F8 + G6 + K4: + K4: | 2,6 | Σ 3,6 | STF 528 | 04226+2538 | 91 | [213] (U, S, M) | |
2 (Ba,Bb/Bc) | SB | 8,5 | . | – | – | 9,4 a | F8 + G6 | K4: + K4: | Σ 2,2 | Σ 1,4 | ||||||
3 (Ba/Bb) | SB | 8,5 | . | – | – | 17,6 d | F8 | G6 | 1,2 | 1,0 | ||||||
Tau | 7 Tau | 1 (AB/C) | V | 5,9 | 9,9 | 22,4″ | 2014 | A3 V + A3 V | Σ 4,7 | STF 412 | 03344+2428 | 130 | [13] (S), [11] (M) | |||
2 (A/B) | V | 6,6 | 6,8 | 0,8″ | 2019 | 520 a | A3 V | A3 V | 2,4 | 2,3 | STF 412 | |||||
Tau | 19 Tau (Taygeta) | SB/A | 4,6 | 6,1 | – | – | 2,0 a | B6 IV | OCC 235 | 03453+2428 | 130 | |||||
Tau | 27 Tau (Atlas) | I/SB | 3,8 | 5,5 | – | – | 291 d | B8 III | 4,7 | 3,4 | MKT 12 | 03492+2403 | 130 | [214] (M, d) | ||
Tau | 28 Tau (Pleione) | SI/SB | 5,1 | . | 0,2″ | 1991 | 218 d | B8 Vne | 2,9 | < 0,4 | CHR 125 | 03492+2408 | 130 | [215] (U, M) | ||
Tau | 30 Tau | V | 5,1 | 9,8 | 9,2″ | 2015 | B3 V | F3 Vn | STF 452 | 03483+1109 | 130 | |||||
Tau | 31 Tau | V | 6,3 | 6,6 | 0,8″ | 2019 | 870 a | KUI 15 | 03520+0632 | 220 | ||||||
Tau | 36 Tau | SI/SB | 5,5 | 5,5 | 0,0″ | 2014 | 7,9 a | K1 II | B7,5 IV: | MCA 13 | 04044+2406 | 340 | ||||
Tau | 46 Tau | V/SB | 5,7 | 6,7 | 0,1″ | 2020 | 7,2 a | F3 V | F3 V | 1,4 ± 0,3 | 0,8 ± 0,2 | A 1938 | 04136+0743 | 40 | [24] (S), [9] (M) | |
Tau | 47 Tau | V | 5,1 | 7,3 | 1,3″ | 2016 | 480 a | G5 III | A7 V: | BU 547 | 04139+0916 | 100 | ||||
Tau | 51 Tau | SI/SB | 5,6 | 8,1 | 0,2″ | 2005 | 11,4 a | A8 V | G0 V | 1,9 ± 0,2 | 1,6 ± 0,2 | MCA 14 | 04184+2135 | 57 | [1] (S, M, d) | |
Tau | 55 Tau | V | 7,3 | 8,6 | 0,6″ | 2018 | 90 a | F7 V | G6 V | STT 79 | 04199+1631 | 47 | [24] (S) | |||
Tau | 62 Tau | CPM | 6,4 | 7,9 | 29,1″ | 2019 | B | A0 V | STF 534 | 04240+2418 | 220 | |||||
Tau | 66 Tau | V | 5,8 | 5,9 | 0,3″ | 2018 | 55 a | A0 | A1 | Σ ≈ 5 | HU 304 | 04239+0928 | 120 | [12] (S, M) | ||
Tau | 70 Tau | SI/SB | 7,0 | 7,7 | 0,1″ | 2018 | 6,3 a | F7 V | F | 1,4 | 1,3 | FIN 342 | 04256+1556 | 47 | [216] (S, M, d) | |
Tau | 80 Tau | V | 5,7 | 8,1 | 1,4″ | 2018 | 173 a | A8 V | G2 V | STF 554 | 04301+1538 | 46 | [24] (S) | |||
Tau | 88 Tau | 1 (A/B) | CPM | 4,3 | 7,8 | 69,2″ | 2017 | A6m + F5 + G2–3 + G2–3 | F8 V + M: | Σ 5,6 | Σ > 1,4 | SHJ 45 | 04357+1010 | 53 | [217] (UAa1/Aa2, UAb1/Ab2, SAa1/Aa2, SAb1/Ab2, MAa1/Aa2, MAb1/Ab2), [218] (UBa/Bb, SBa/Bb, MBa/Bb) | |
2 (Aa/Ab) | SI | 4,4 | 6,6 | 0,2″ | 2019 | 18,0 a | A6m + F5 | G2–3 + G2–3 | Σ 3,5 | Σ 2,1 | CHR 18 | |||||
2 (Ba/Bb) | SB | 7,8 | . | – | – | 3,7 a | F8 V | M: | 1,2 | > 0,15 | ||||||
3 (Aa1/Aa2) | SB/A | 4,4 | . | – | – | 3,57 d | A6m | F5 | 2,1 | 1,4 | ||||||
3 (Ab1/Ab2) | SB/A | 6,6 | . | – | – | 7,89 d | G2–3 | G2–3 | 1,1 | 1,0 | ||||||
Tau | 104 Tau | V | 5,8 | 5,8 | 0,1″ | 1988 | 1,2 a | G4 V | G4 V | 1,0 | 1,0 | A 3010 | 05074+1839 | 16 | [24] (S), [11] (M) | |
Tau | 108 Tau | V | 6,3 | 12,5 | 1,9″ | 2004 | COU 158 | 05155+2217 | 160 | |||||||
Tau | 115 Tau | 1 (A/BC) | V | 5,4 | 10,6 | 10,1″ | 2016 | STT 107 | 05272+1758 | 200 | ||||||
2 (B/C) | V | 11,1 | 11,8 | 7,0″ | 2015 | STT 107 | ||||||||||
3 (Aa/Ab) | SI | 5,8 | 6,8 | 0,1″ | 2020 | 15,9 a | MCA 19 | |||||||||
Tau | 118 Tau | 1 (A/B) | V | 5,8 | 6,7 | 4,6″ | 2020 | B8,5 V | A0 Vn | STF 716 | 05293+2509 | 130 | ||||
2 (Aa/Ab) | V(aO) | 5,8 | 12,1 | 1,8″ | 2003 | RBR 1 | ||||||||||
2 (Ba/Bb) | V(aO) | 6,7 | 10,1 | 1,0″ | 2003 | RBR 1 | ||||||||||
Tau | 126 Tau | V | 5,0 | 6,6 | 0,2″ | 2011 | 111 a | B8 | B7 | Σ ≈ 9 | BU 1007 | 05413+1632 | 190 | [12] (S, M) | ||
Tau | 131 Tau | SI | 6,2 | 6,9 | 0,2″ | 2016 | CHR 160 | 05472+1429 | 100 | |||||||
Tau | V711 Tau | 1 (A/B) | V | 6,0 | 8,9 | 6,7″ | 2016 | 1210 a | F8 V + G5 V | K4 V + K8 V | Σ 2,0 | Σ 1,3 | STF 422 | 03368+0035 | 30 | [3] (UAa/Ab, UBa/Bb), [2] (S, M) |
2 (Aa/Ab) | SB | 6,0 | . | – | – | 2,84 d | F8 V | G5 V | 1,1 | 0,9 | ||||||
2 (Ba/Bb) | SB | 8,9 | . | – | – | 3,2 a | K4 V | K8 V | 0,7 | 0,6 | ||||||
Tau | HR 1188 | V | 5,7 | 6,5 | 0,4″ | 2017 | 61 a | A2 V | A5 V | Σ 4,2 ± 0,4 | STT 65 | 03503+2535 | 56 | [13] (S), [58] (M) | ||
Tau | HR 1902 | V | 6,5 | 6,6 | 1,1″ | 2019 | 770 a | B8 IV | B8 IV | Σ 3,4 | STF 749 | 05371+2655 | 150 | [24] (S), [219] (M) | ||
Tau | HR 1997 | V | 6,3 | 7,6 | 0,1″ | 2018 | 230 a | B9 Vn | 2,7 | 2,0 | STT 118 | 05484+2052 | 200 | [90] (S, M) | ||
Tel | HR 7549 | V | 5,8 | 6,4 | 23,0″ | 2015 | A1–3 V | G8–K0 III | DUN 227 | 19526-5458 | 130 | |||||
Tri | β Tri | I/SB | 3,6 | 4,0 | – | – | 31,4 d | A5 III | 3,5 ± 0,3 | 1,4 ± 0,1 | MKT 4 | 02095+3459 | 41 | [1] (S, M, d) | ||
Tri | δ Tri | I/SB | 5,0 | 6,9 | – | – | 10,0 d | G0,5 VFe | K: | 1,0 | 0,7 | MKT 5 | 02171+3413 | 11,0 | [18] (M) | |
Tri | ε Tri | V | 5,4 | 11,4 | 4,2″ | 1990 | STF 201 | 02030+3317 | 110 | |||||||
Tri | ι Tri | 1 (A/B) | V | 5,3 | 6,7 | 4,0″ | 2019 | 5200 a | G0 III + G5 III | F5 V | STF 227 | 02124+3018 | 89 | [3] (UAa/Ab, UBa/Bb) | ||
2 (Aa/Ab) | SB | 5,3 | . | – | – | 14,7 d | G0 III | G5 III | ||||||||
2 (Ba/Bb) | SB | 6,7 | . | – | – | 2,24 d | F5 V | |||||||||
Tuc | α Tuc | SB/A | 2,9 | . | – | – | 11,5 a | alp Tuc | 22185-6016 | 61 | ||||||
Tuc | β Tuc | 1 (β1/2 = ABCD / β3 = E) | CPM | 3,6 | 5,1 | 548,9″ | 2000 | B9,5 Va + A3 IV + A7 V | A0 V | SHY 114 | 00315-6257 | 41 | ||||
2 (β1 = AB / β2 = CD) | V | 4,3 | 4,5 | 27,2″ | 2017 | B9,5 Va | A3 IV + A7 V | LCL 119 | ||||||||
2 (Ea/Eb) | V | 5,8 | 6,0 | 0,1″ | 1964 | A0 V | B 8 | |||||||||
3 (A/B) | V | 4,4 | 13,5 | 2,6″ | 1932 | B9,5 Va | B 7 | |||||||||
3 (C/D) | V | 4,6 | 6,5 | 0,4″ | 2017 | 44,7 a | A3 IV | A7 V | I 260 | |||||||
Tuc | κ Tuc | 1 (AB/CD) | CPM | 4,8 | 7,2 | 319,2″ | 2010 | ≈ 300 000 a | F6 IV + G5 V | K2 V + K3 V | Σ 2,4 | Σ 1,7 | HJ 3423 | 01158-6853 | 21 | [201] (UAB/CD, UAa/Ab, S, M) |
2 (A/B) | V | 4,9 | 7,5 | 4,6″ | 2017 | 1200 a | F6 IV | G5 V | Σ 1,5 | 0,9 | HJ 3423 | |||||
2 (C/D) | V | 7,8 | 8,3 | 1,0″ | 2018 | 85 a | K2 V | K3 V | 0,9 | 0,8 | I 27 | |||||
3 (Aa/Ab) | A | 4,9 | . | – | – | 22? a | F6 IV | 1,3 | 0,2? | |||||||
Tuc | λ1 Tuc | V | 6,7 | 7,4 | 20,4″ | 2015 | 580 000 a | F7 IV–V | G0–2 V | DUN 2 | 00524-6930 | 61 | ||||
UMa | α UMa (Dubhe) | 1 (AB/C) | CPM | 1,8 | 7,2 | 370,0″ | 2015 | K1 II–III + F0 V | F7 V | Σ ≈ 6 | BU 1077 | 11037+6145 | 38 | [24] (SA/B), [220] (M), [221] (UCa/Cb) | ||
2 (A/B) | V/SB | 2,0 | 5,0 | 0,8″ | 2017 | 44 a | K1 II–III | F0 V | 4,3 ± 0,3 | ≈ 1,6 | BU 1077 | |||||
2 (Ca/Cb) | SB | 7,2 | . | – | – | 6,04 d | F7 V | – | ||||||||
UMa | γ UMa (Phecda) | A | 2,4 | . | – | – | 20,5 a | A0 Ve | K2 V | 2,9 | 0,8 | gam UMa | 11538+5342 | 26 | [148] (S, M) | |
UMa | ζ UMa / 80 UMa (Mizar/Alkor) | 1 (ζ1/2 = AB / 80 = C) | CPM | 2,0 | 4,0 | 707,7″ | 2017 | A2 V + A2 V + kA1h(eA)mA7 IV–V | A5 Vn + M2 V | Σ ≈ 7,2 | Σ 2,1 | STF 1744 | 13239+5456 | 25 | [33] (SAa/Ab, MAa/Ab, d), [18] (MBa/Bb), [3] (UBa/Bb), [222] (UCa/Cb, SCa/Cb, MCa/Cb) | |
2 (ζ1 = A / ζ2 = B) | V | 2,3 | 3,9 | 14,6″ | 2019 | A2 V + A2 V | kA1h(eA)mA7 IV–V | Σ 4,9 | Σ ≈ 2,3 | STF 1744 | ||||||
2 (Ca/Cb) | V(IR) | 4,0 | > 8 | 1,0″ | 2009 | ≈ 100 a | A5 Vn | M2 V | 1,8 | 0,3 | PSF 1 | |||||
3 (Aa/Ab) | I/SB | 3,0 | 3,0 | – | – | 20,5 d | A2 V | A2 V | 2,5 | 2,4 | PEA 1 | |||||
3 (Ba/Bb) | SB | 3,9 | . | – | – | 176 d | kA1h(eA)mA7 IV–V | 1,8 | ≈ 0,2–0,7 | |||||||
UMa | ι UMa | 1 (A/BC) | V | 3,1 | 9,2 | 2,4″ | 2017 | 490 a | F0 IV–V + D: | M3 V + M4 V | Σ 2,7 ± 0,4 | Σ 0,7 | HJ 2477 | 08592+4803 | 15 | [223] (UAa/Ab, S, M) |
2 (Aa/Ab) | SB | 3,1 | . | – | – | 12,2 a | F0 IV–V | D: | 1,7 ± 0,1 | 1,0 ± 0,3 | ||||||
2 (B/C) | V | 9,9 | 10,1 | 0,9″ | 2017 | 39 a | M3 V | M4 V | 0,4 | 0,3 | HU 628 | |||||
UMa | κ UMa | V | 4,2 | 4,5 | 0,3″ | 2019 | 35,6 a | A0 IV–V | A0 V | Σ 6,3 ± 1,0 | A 1585 | 09036+4709 | 110 | [24] (S), [9] (M) | ||
UMa | μ UMa | SB/A | 3,1 | . | – | – | 230 d | M0 III | 2,2 | ≈ 1,6 | mu UMa | 10223+4130 | 71 | [224] (S, M) | ||
UMa | ν UMa | V | 3,6 | 10,1 | 7,0″ | 2020 | STF 1524 | 11185+3306 | 120 | |||||||
UMa | ξ UMa | 1 (A/B) | V | 4,3 | 4,8 | 2,1″ | 2019 | 59,9 a | F8,5: V + M: | G2 V + M: | Σ 1,4 | Σ 1,0 | STF 1523 | 11182+3132 | 8,8 | [3] (UAa/Ab, UBa/Bb), [18] (SAb, SBb, M) |
2 (Aa/Ab) | SB | 4,3 | . | – | – | 1,8 a | F8,5: V | M: | 1,0 | 0,4 | ||||||
2 (Ba/Bb) | SB | 4,8 | . | – | – | 3,98 d | G2 V | M: | 0,9 | 0,1 | ||||||
UMa | σ2 UMa | V | 4,9 | 8,9 | 4,3″ | 2016 | 920 a | F6 IV–V | K2 V | 1,3 | ≈ 0,7 | STF 1306 | 09104+6708 | 20 | [24] (S), [18] (M) | |
UMa | φ UMa | V | 5,3 | 5,4 | 0,4″ | 2019 | 105 a | A3 IV | A3 IV | STT 208 | 09521+5404 | 160 | [24] (S) | |||
UMa | 16 UMa | SB/A | 5,2 | 8,9 | – | – | 16,2 d | G0 V | M: | 1,1 | 0,6 | 16 UMa | 09143+6125 | 20 | [18] (S2, M) | |
UMa | 55 UMa | 1 (A/B) | SI | 4,8 | 5,3 | 0,1″ | 2007 | 5,1 a | A1 V + A2 V | A1 V | Σ 3,8 | 2,1 | CHR 133 | 11191+3811 | 60 | [225] (UAa/Ab, S, M) |
2 (Aa/Ab) | SB | 4,8 | . | – | – | 2,55 d | A1 V | A2 V | 2,0 | 1,8 | ||||||
UMa | 62 UMa | SI/SB | 5,7 | 6,7 | 0,0″ | 2015 | 268 d | F5 | 1,3 | 1,2 | BNU 3 | 11416+3145 | 41 | [226] (M) | ||
UMa | 65 UMa | 1 (ABC/D) | CPM | 6,5 | 7,0 | 62,5″ | 2018 | A3 V + A3 V + A8–9 | A1p + F | STF 1579 | 11551+4629 | 87 | [21] (UAa/Ab, SAa/Ab, SB), [60] (SDa/Db) | |||
2 (AB/C) | V | 6,7 | 8,3 | 3,9″ | 2019 | A3 V + A3 V + A8–9 | STF 1579 | |||||||||
2 (Da/Db) | SI | 7,1 | 9,2 | 0,1″ | 2018 | A1p | F | BAG 46 | ||||||||
3 (A/B) | V | 6,5 | 9,2 | 0,3″ | 2019 | 118 a | A3 V + A3 V | A8–9 | A 1777 | |||||||
4 (Aa/Ab) | E/SB | 6,5 | . | – | – | 1,73 d | A3 V | A3 V | ||||||||
UMa | 78 UMa | V | 5,0 | 7,9 | 0,7″ | 2019 | 105 a | F1 V | G6 V | BU 1082 | 13007+5622 | 25 | [24] (S) | |||
UMa | HR 4098 | V | 6,4 | 12,6 | 4,0″ | 2015 | 81 a | KUI 50 | 10281+4847 | 23 | ||||||
UMa | HR 4439 | V | 5,7 | 7,6 | 0,9″ | 2017 | 73 a | F4 V | G3 V | 1,3 | 0,9 | STT 235 | 11323+6105 | 29 | [24] (S), [11] (M) | |
UMa | HR 4486 | V | 6,5 | 8,2 | 8,9″ | 2019 | 1580 a | G0 V | K2 V | STF 1561 | 11387+4507 | 23 | ||||
UMa | W UMa | 1 (A/B) | V | 8,0 | 12,4 | 6,4″ | 2019 | F8 V + F8 V | Σ 1,7 | ES 1825 | 09438+5557 | 52 | [3] (U, S), [227] (M) | |||
2 (Aa/Ab) | E/SB | 7,9 | . | – | – | 0,33 d | F8 V | F8 V | 1,1 | 0,6 | ||||||
UMa | Gliese 338 | V | 7,8 | 7,9 | 16,9″ | 2019 | 980 a | K7 V | M0 V | STF 1321 | 09144+5241 | 6,3 | ||||
UMa | Gliese 412 | CPM | 8,8 | 14,6 | 32,0″ | 2017 | M1 Ve | M6 V | VBS 18 | 11055+4332 | 4,8 | |||||
UMa | Winnecke 4 (M 40) | O | 9,7 | 10,2 | 53,2″ | 2017 | G0 | F8 | WNC 4 | 12222+5805 | 320 | |||||
UMi | α UMi (Polarstern) | 1 (A/B) | V | 2,0 | 9,1 | 18,4″ | 2016 | F8 Ib + A5 | F3 V | Σ 5,1 ± 1,3 | ≈ 1,4 | STF 93 | 02318+8916 | 130 | [3] (SAa/Ab), [228] (M) | |
2 (Aa/Ab) | SI/SB | 2,3 | 4,3 | 0,1″ | 2014 | 29,6 a | F8 Ib | A5 | 3,5 ± 0,8 | 1,6 ± 0,5 | WRH 39 | |||||
UMi | π2 UMi | V | 7,3 | 8,2 | 0,7″ | 2013 | 172 a | STF 1989 | 15396+7959 | 120 | ||||||
Vel | γ Vel | 1 (γ2 = A / γ1 = B) | CPM | 1,8 | 4,1 | 41,2″ | 2017 | WC8 + O7,5 III–V | B2 III | Σ 37,5 ± 1,7 | DUN 65 | 08095-4720 | 340 | [229] (U, M, d) | ||
2 (γ2 Vel A/B) | SB | 1,8 | . | – | – | 78,5 d | WC8 | O7,5 III–V | 9,0 ± 0,6 | 28,5 ± 1,1 | ||||||
Vel | δ Vel | 1 (A/B) | V | 2,0 | 5,6 | 0,8″ | 2019 | 147 a | A2 IV + A4 V | F8 V | Σ 4,7 | 1,4 | I 10 | 08447-5443 | 25 | [230] (M, d) |
2 (Aa/Ab) | E/I/SB | 2,0 | . | – | – | 45,2 d | A2 IV | A4 V | 2,4 | 2,3 | KEL 1 | |||||
Vel | μ Vel | V | 2,8 | 5,7 | 2,3″ | 2019 | 143 a | G5 III | G2 V | R 155 | 10468-4925 | 36 | [24] (S) | |||
Vel | ψ Vel | V | 3,9 | 5,1 | 1,0″ | 2019 | 34,1 a | F3 IV | F0 IV | COP 1 | 09307-4028 | 19 | [13] (S) | |||
Vel | B Vel | V | 5,1 | 6,1 | 0,9″ | 2008 | I 67 | 08225-4829 | 530 | |||||||
Vel | p Vel | 1 (A/B) | V | 4,1 | 5,8 | 0,1″ | 2019 | 16,7 a | F3 IV + F0 V | A6 V | Σ 3,9 | 2,4 | SEE 119 | 10373-4814 | 27 | [231] (UAa/Ab, S, M) |
2 (Aa/Ab) | SB | 4,1 | . | – | – | 10,2 d | F3 IV | F0 V | 2,1 | 1,8 | ||||||
Vel | s Vel | V | 5,6 | 6,0 | 13,2″ | 2010 | B8–A0 | B8 II: | PZ 3 | 10320-4504 | 260 | |||||
Vel | 33 G. Vel | 1 (A/B) | V | 5,5 | 7,2 | 3,5″ | 2008 | B1,5 V | B4 V | HJ 4104 | 08291-4756 | 480 | ||||
2 (Aa/Ab) | SI | 5,9 | 6,4 | 0,1″ | 2018 | 340 a | B1,5 V | FIN 315 | ||||||||
Vel | HR 3817 | V | 5,5 | 6,2 | 2,0″ | 2008 | HJ 4220 | 09337-4900 | 250 | |||||||
Vel | HR 3840 | V | 6,1 | 6,3 | 0,7″ | 2015 | SEE 115 | 09372-5340 | 72 | |||||||
Vel | HR 3976 | V | 5,3 | 7,1 | 1,0″ | 2019 | 187 a | K1 IV | G5 V | I 173 | 10062-4722 | 74 | [24] (S) | |||
Vel | Luhman 16 | V(aO) | 16,2 | . | 0,3″ | 2016 | 27,4 a | L7,5 | T0,5 | 0,03 | 0,03 | LUH 16 | 10493-5319 | 2,0 | [30] (V), [232] (S, M, d) | |
Vir | α Vir (Spica) | SB | 1,3 | 4,5 | – | – | 4,01 d | B1 III–IV | B2 V | 11,4 ± 1,2 | 7,2 ± 0,8 | OCC 418 | 13252-1110 | 77 | [13] (S), [233] (M) | |
Vir | γ Vir (Porrima) | V | 3,5 | 3,5 | 2,5″ | 2020 | 169 a | F0 V | F0 V | 1,4 | 1,4 | STF 1670 | 12417-0127 | 12,1 | [13] (S), [234] (M, d) | |
Vir | η Vir | 1 (A/B) | SI | 3,9 | 5,9 | 0,1″ | 2020 | 13,1 a | A2 IV + A8–F0 V | – | Σ 4,4 | 1,7 | MCA 37 | 12199-0040 | 79 | [235][236] (UAa/Ab, S, M) |
2 (Aa/Ab) | SB | 3,9 | . | – | – | 71,8 d | A2 IV | A8–F0 V | 2,5 | 1,9 | ||||||
Vir | θ Vir | 1 (A/B) | V | 4,4 | 9,4 | 7,0″ | 2015 | STF 1724 | 13099-0532 | 83 | ||||||
2 (Aa/Ab) | SI | 4,5 | 6,8 | 0,4″ | 2019 | 700 a | MCA 38 | |||||||||
Vir | ι Vir | A | 4,1 | . | – | – | 55 a | iot Vir | 14160-0600 | 22 | ||||||
Vir | λ Vir | I/SB | 4,5 | . | – | – | 207 d | A1m | A1m | 1,9 | 1,7 | IOT 1 | 14191-1322 | 53 | [33] (S, M) | |
Vir | φ Vir | V | 4,9 | 10,0 | 4,8″ | 2015 | G2 III | G4 V | STF 1846 | 14282-0214 | 37 | [24] (S) | ||||
Vir | 46 Vir | V | 6,2 | 8,8 | 0,6″ | 2016 | 900 a | AGC 5 | 13006-0322 | 100 | ||||||
Vir | 48 Vir | V | 7,1 | 7,7 | 0,4″ | 2018 | 440 a | BU 929 | 13039-0340 | 160 | ||||||
Vir | 54 Vir | V | 6,8 | 7,2 | 5,4″ | 2018 | B9 V | A2 VpSr | SHJ 151 | 13134-1850 | 190 | |||||
Vir | 84 Vir | V | 5,6 | 8,3 | 2,7″ | 2015 | G8 III | G3 IV | STF 1777 | 13431+0332 | 73 | |||||
Vir | 86 Vir | 1 (AB/CD) | CPM | 5,6 | 11,9 | 27,3″ | 2000 | STF 1780 | 13459-1226 | 110 | ||||||
2 (A/B) | V | 5,7 | 8,5 | 1,0″ | 2001 | BU 935 | ||||||||||
2 (C/D) | V | 11,9 | 13,1 | 2,4″ | 1958 | STF 1780 | ||||||||||
Vir | HR 4935 | V | 6,3 | 6,5 | 0,2″ | 2020 | 59 a | BU 341 | 13038-2035 | 28 | ||||||
Vir | HR 5106 | V | 6,3 | 7,3 | 0,4″ | 2019 | 178 a | BU 932 | 13347-1313 | 150 | ||||||
Vir | Wolf 424 | V | 12,6 | 12,6 | 0,7″ | 2020 | 15,8 a | M5,5 V | M7 V | 0,14 | 0,13 | REU 1 | 12335+0901 | 4,4 | [40] (S), [237] (M) | |
Vol | γ Vol | V | 3,9 | 5,4 | 14,2″ | 2020 | K0 III | F0–3 | DUN 42 | 07087-7030 | 40 | |||||
Vol | ε Vol | 1 (A/B) | V | 4,4 | 7,3 | 5,7″ | 2020 | RMK 7 | 08079-6837 | 230 | [3] (U) | |||||
2 (Aa/Ab) | SB | 4,4 | . | – | – | 14,2 d | ||||||||||
Vol | ζ Vol | V | 4,0 | 9,3 | 16,0″ | 2020 | DUN 57 | 07418-7236 | 43 | |||||||
Vol | κ Vol | 1 (κ1/2 = AB / C) | CPM | 4,7 | 7,7 | 98,4″ | 2020 | B9 III–IV + B9–A0 IV | BSO 17 | 08198-7131 | 130 | |||||
1 (κ1 = A / κ2 = B) | CPM | 5,3 | 5,6 | 64,0″ | 2020 | B9 III–IV | B9–A0 IV | BSO 17 | ||||||||
Vul | 2 Vul | V | 5,4 | 8,8 | 1,8″ | 2015 | BU 248 | 19177+2302 | 570 | |||||||
Vul | 13 Vul | V | 4,6 | 7,4 | 1,4″ | 2016 | 620 a | DJU 4 | 19535+2405 | 95 | ||||||
Vul | 16 Vul | V | 5,8 | 6,2 | 0,7″ | 2019 | 1200 a | STT 395 | 20020+2456 | 68 | ||||||
Vul | 23 Vul | SI | 4,8 | 6,5 | 0,0″ | 2007 | 25,3 a | CHR 94 | 20158+2749 | 100 |
Häufige Entdeckercodes
Nachfolgend findet sich eine Auswahl der Bedeutung von einigen häufigen Entdeckercodes:
- A – Robert Grant Aitken
- AC – Alvan Clark
- AGC – Alvan Graham Clark
- B – Willem Hendrik van den Bos
- BU – Sherburne Wesley Burnham
- CHR – Center for High Angular Resolution Astronomy
- DJU – Petar Đurković
- DUN – James Dunlop
- FIN – William Stephen Finsen
- H – Friedrich Wilhelm Herschel
- I – Robert Thorburn Ayton Innes
- HDS – Hipparcos Double Star
- HJ – John Frederick William Herschel
- HU – William Joseph Hussey
- KUI – Gerard Peter Kuiper
- MCA – Harold A. McAlister
- MKT – Mark III Stellar Interferometer
- NOI – Navy Precision Optical Interferometer
- SEE – Thomas Jefferson Jackson See
- SHJ – James South & John Frederick William Herschel
- STF (auch Σ) – Friedrich Georg Wilhelm Struve
- STFA (auch ΣA) – Friedrich Georg Wilhelm Struve (Addendum)
- STT (auch OΣ) – Otto Wilhelm von Struve
- TOK – Andrei A. Tokovinin
- WRH – Raymond H. Wilson, Jr.
Quellen
Allgemeine Quellen
Solange in der Spalte „Quelle“ nichts anderes angegeben ist, stammen:
- die Helligkeiten (V1, V2), Abstände (ρ) und Epochen (Ep.) aus dem Washington Double Star Catalog (Vers. 2021-08-09),
- die Umlaufzeiten aus dem 6th Orbit Catalog (Last Update 2021-08-02),
- die Spektralklassen aus der SIMBAD-Datenbank,
- die Entfernungen von der in der SIMBAD-Datenbank hinterlegten Parallaxe (meistens aus den Katalogen Hipparcos, the New Reduction (van Leeuwen 2007) und Gaia DR2 (Gaia Collaboration 2018)).
Einzelnachweise
Alle Massen und alle nicht aus den allgemeinen Quellen entnommenen Daten stammen aus folgenden Quellen:
- ↑ a b c d e f g h i Dimitri Pourbaix: Resolved double-lined spectroscopic binaries: A neglected source of hypothesis-free parallaxes and stellar masses. In: Astronomy & Astrophysics Supplement Series. Bd. 145, 2000, S. 215–222, bibcode:2000A&AS..145..215P, doi:10.1051/aas:2000237.
- ↑ a b c d e f g h i j k l José A. Docobo, Manuel Andrade: A Methodology for the Description of Multiple Stellar Systems with Spectroscopic Subcomponents. In: The Astrophysical Journal. Bd. 652 (1), 2006, S. 681–695, bibcode:2006ApJ...652..681D, doi:10.1086/508053.
- ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi Dimitri Pourbaix et al.: 9th Catalogue of Spectroscopic Binary Orbits. VizieR-Datenkatalog B/sb9 (elektronisch veröffentlicht). 2009, bibcode:2009yCat....102020P.
- ↑ Michael Bottom et al.: Resolving the Delta Andromedae Spectroscopic Binary with Direct Imaging. In: The Astrophysical Journal. Bd. 809 (1), 2015, Artikel-ID 11, bibcode:2015ApJ...809...11B, doi:10.1088/0004-637X/809/1/11, arxiv:1506.07517.
- ↑ a b c d e f g h i j k l m Peter P. Eggleton, Kadri Yakut: Models for Sixty Double-Lined Binaries containing Giants. In: Monthly Notices of the Royal Astronomical Society. Bd. 468 (3), 2017, S. 3533–3556, bibcode:2017MNRAS.468.3533E, doi:10.1093/mnras/stx598, arxiv:1611.05041.
- ↑ G. M. Hill et al.: Omicron Andromedae is Quadruple. In: Publications of the Astronomical Society of the Pacific. Bd. 100, 1988, S. 243–250, bibcode:1988PASP..100..243H, doi:10.1086/132161.
- ↑ R. Ya. Zhuchkov et al.: Physical parameters and dynamical properties of the multiple star o And. In: Astronomy Reports. Bd. 54 (12), 2010, S. 1134 ff., bibcode:2010ARep...54.1134Z, doi:10.1134/S1063772910120061.
- ↑ Christian A. Hummel et al.: Orbits of Small Angular Scale Binaries Resolved with the Mark III Interferometer. In: The Astronomical Journal. Bd. 110, 1995, 376–390, bibcode:1995AJ....110..376H, doi:10.1086/117528.
- ↑ a b c d e f g h i j k Matthew W. Muterspaugh et al.: The Phases Differential Astrometry Data Archive. II. Updated Binary Star Orbits and a Long Period Eclipsing Binary. In: The Astronomical Journal. Bd. 140 (6), S. 1623–1630, bibcode:2010AJ....140.1623M, doi:10.1088/0004-6256/140/6/1623, arxiv:1010.4043.
- ↑ a b Christopher D. Farrington et al.: Separated Fringe Packet Observations with the CHARA Array. II. ω Andromeda, HD 178911, and ξ Cephei. In: The Astronomical Journal. Bd 148 (3), 2014, Artikel-ID 48, bibcode:2014AJ....148...48F, doi:10.1088/0004-6256/148/3/48, arxiv:1407.0639.
- ↑ a b c d e f g h i j k l m n o p q r s t u Z. Cvetković, S. Ninković: Masses of visual binaries. VizieR-Datenkatalog J/other/Ser/180.71 (elektronisch veröffentlicht). 2011, bibcode:2011yCatp042018001C.
- ↑ a b c d e Theo A. ten Brummelaar et al.: Binary Star Differential Photometry Using the Adaptive Optics System at Mount Wilson Observatory. In: The Astronomical Journal. Bd. 119 (5), 2000, S. 2403–2414, bibcode:2000AJ....119.2403T, doi:10.1086/301338.
- ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad Dorrit Hoffleit, Wayne H. Warren, Jr.: Bright Star Catalogue, 5th Revised Ed. VizieR-Datenkatalog V/50 (elektronisch veröffentlicht). 1995, bibcode:1995yCat.5050....0H. Die Spektralklassen stammen entweder direkt aus dem Katalog oder aus dem Bereich Note/Remarks.
- ↑ Jesus Maldonado et al.: HADES RV Programme with HARPS-N at TNG. III. Flux-flux and activity-rotation relationships of early-M dwarfs. In: Astronomy & Astrophysics. Bd. 598, 2017, Artikel-ID A27, bibcode:2017A&A...598A..27M, doi:10.1051/0004-6361/201629223, arxiv:1610.05906.
- ↑ Matteo Pinamonti et al.: The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: a multiple wide planetary system sculpted by binary interaction. In: Astronomy & Astrophysics. Bd. 617, 2018, Artikel-ID A104, bibcode:2018A&A...617A.104P, doi:10.1051/0004-6361/201732535, arxiv:1804.03476.
- ↑ a b c d e f José A. Docobo, Manuel Andrade: Dynamical and physical properties of 22 binaries discovered by W. S. Finsen. In: Monthly Notices of the Royal Astronomical Society. Bd. 428 (1), 2013, S. 321–339, bibcode:2013MNRAS.428..321D, doi:10.1093/mnras/sts045.
- ↑ Sandy K. Leggett et al.: The Physical Properties of Four ~600 K T Dwarfs. In: The Astrophysical Journal. Bd. 695 (2), 2009, S. 1517–1526, bibcode:2009ApJ...695.1517L, doi:10.1088/0004-637X/695/2/1517, arxiv:0901.4093.
- ↑ a b c d e f g h i j k Klaus Fuhrmann: Nearby stars of the Galactic disc and halo – IV. In: Monthly Notices of the Royal Astronomical Society. Bd. 384 (1), 2008, S. 173–224, bibcode:2008MNRAS.384..173F, doi:10.1111/j.1365-2966.2007.12671.x.
- ↑ a b c Nancy Remage Evans et al.: Binary Cepheids: Separations and Mass Ratios in 5 M⊙ Binaries. In: The Astronomical Journal. Bd. 146 (4), 2013, Artikel-ID 93, bibcode:2013AJ....146...93E, doi:10.1088/0004-6256/146/4/93, arxiv:1307.7123.
- ↑ a b c d e Brian D. Mason et al.: Binary Star Orbits. IV. Orbits of 18 Southern Interferometric Pairs. In: The Astronomical Journal. Bd. 140 (3), 2010, S. 735–743, bibcode:2010AJ....140..735M, doi:10.1088/0004-6256/140/3/735.
- ↑ a b c d e f g h i j k l m Petr Zasche et al.: A Catalog of Visual Double and Multiple Stars With Eclipsing Components. In: The Astronomical Journal. Bd. 138 (2), 2009, S. 664–679, bibcode:2009AJ....138..664Z, doi:10.1088/0004-6256/138/2/664, arxiv:0907.5172.
- ↑ Jeffrey L. Linsky et al.: Stellar Activity at the End of the Main Sequence: GHRS Observations of the M8 Ve Star VB 10. In: The Astrophysical Journal. Bd. 455, 1995, S. 670–676, bibcode:1995ApJ...455..670L, doi:10.1086/176614.
- ↑ Olivier Absil et al.: Searching for faint companions with VLTI/PIONIER. I. Method and first results. In: Astronomy & Astrophysics. Bd. 535, 2011, Artikel-ID A68, bibcode:2011A&A...535A..68A, doi:10.1051/0004-6361/201117719, arxiv:1110.1178.
- ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv Terry W. Edwards: MK classification for visual binary components. In: The Astronomical Journal. Bd. 81, 1976, S. 245–249, bibcode:1976AJ.....81..245E, doi:10.1086/111879.
- ↑ Andrei A. Tokovinin: The Triple System Zeta Aquarii. In: The Astrophysical Journal. Bd. 831 (2), 2016, Artikel-ID 151, bibcode:2016ApJ...831..151T, doi:10.3847/0004-637X/831/2/151, arxiv:1608.08564.
- ↑ Ellyn K. Baines et al.: Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer. In: The Astronomical Journal. Bd. 155 (1), 2018, Artkikel-ID 30, bibcode:2018AJ....155...30B, doi:10.3847/1538-3881/aa9d8b, arxiv:1712.08109.
- ↑ a b Rene A. Mendez et al.: Orbits for 18 Visual Binaries and Two Double-line Spectroscopic Binaries Observed with HRCAM on the CTIO SOAR 4 m Telescope, Using a New Bayesian Orbit Code Based on Markov Chain Monte Carlo. In: The Astronomical Journal. Bd. 154 (5), 2017, Artikel-ID 187, bibcode:2017AJ....154..187M, doi:10.3847/1538-3881/aa8d6f, arxiv:1709.06582.
- ↑ Andrei A. Tokovinin: New Orbits Based on Speckle Interferometry at SOAR. II. In: The Astronomical Journal. Bd. 154 (3), 2017, Artikel-ID 110, bibcode:2017AJ....154..110T, doi:10.3847/1538-3881/aa8459, arxiv:1708.01300.
- ↑ José A. Docobo et al.: Visual Orbit and Individual Masses of the Single-lined Spectroscopic Binary 94 AQR A (HD 219834A; MCA 74). In: The Astronomical Journal. Bd. 156 (3), 2018, Artikel-ID 85, bibcode:2018AJ....156...85D, doi:10.3847/1538-3881/aad179.
- ↑ a b c d e f g h i j k V-Helligkeit aus der SIMBAD-Datenbank entnommen.
- ↑ M. Gromadzki, Joanna Mikołajewska: The spectroscopic orbit and the geometry of R Aquarii. In: Astronomy & Astrophysics. Bd. 495 (3), 2009, S. 931–936, bibcode:2009A&A...495..931G, doi:10.1051/0004-6361:200810052, arxiv:0804.4139.
- ↑ Xavier Delfosse et al.: Accurate masses of very low mass stars. II. The very low mass triple system GL 866. In: Astronomy & Astrophysics. Bd. 350, 1999, L39–L42, bibcode:1999A&A...350L..39D, arxiv:astro-ph/9909409.
- ↑ a b c d e f g h i j k l m n o p Guillermo Torres, J. Andersen, A. Giménez: Accurate masses and radii of normal stars: modern results and applications. In: The Astronomy & Astrophysics Review. Bd. 18 (1–2), 2010, S. 67–126, bibcode:2010A&ARv..18...67T, doi:10.1007/s00159-009-0025-1, arxiv:0908.2624.
- ↑ Hicran Bakıș et al.: Active binary R Arae revisited: Bringing the secondary component to light and physical modelling of the circumstellar material. In: Monthly Notices of the Royal Astronomical Society. Bd. 458 (1), 2016, S. 508–516, bibcode:2016MNRAS.458..508B, doi:10.1093/mnras/stw320.
- ↑ Brian D. Mason: Binary Star Orbits from Speckle Interferometry. XI. Orbits of Twelve Lunar Occultation Systems. In: The Astronomical Journal. Bd. 114, 1997, S. 808–818, bibcode:1997AJ....114..808M, doi:10.1086/118514.
- ↑ a b c Matthew W. Muterspaugh et al.: The Phases Differential Astrometry Data Archive. V. Candidate Substellar Companions to Binary Systems. In: The Astronomical Journal. Bd. 140 (6), 2010, S. 1657–1671, bibcode:2010AJ....140.1657M, doi:10.1088/0004-6256/140/6/1657, arxiv:1010.4048.
- ↑ Lewis C. Roberts, Jr. et al.: Know the Star, Know the Planet. III. Discovery of Late-Type Companions to Two Exoplanet Host Stars. In: The Astronomical Journal. Bd. 149 (4), 2015, Artikel-ID 118, bibcode:2015AJ....149..118R, doi:10.1088/0004-6256/149/4/118, arxiv:1503.01211.
- ↑ a b José A. Docobo et al.: Improved orbits and parallaxes for eight visual binaries with unrealistic previous masses using the Hipparcos parallax. In: Monthly Notices of the Royal Astronomical Society. Bd. 459 (2), 2016, S. 1580–1585, bibcode:2016MNRAS.459.1580D, doi:10.1093/mnras/stw709, arxiv:1609.03392.
- ↑ Guillermo Torres et al.: Capella (α Aurigae) Revisited: New Binary Orbit, Physical Properties, and Evolutionary State. In: The Astrophysical Journal. Bd. 807 (1), 2015, Artikel-ID 26, bibcode:2015ApJ...807...26T, doi:10.1088/0004-637X/807/1/26, arxiv:1505.07461.
- ↑ a b c d e Wilhelm Gliese, Hartmut Jahreiß: Preliminary Version of the Third Catalogue of Nearby Stars. VizieR-Datenkatalog V/70A (elektronisch veröffentlicht). 1991, bibcode:1991adc..rept.....G.
- ↑ Donald W. Hoard et al.: Taming the Invisible Monster: System Parameter Constraints for epsilon Aurigae from the Far-ultraviolet to the Mid-infrared. In: The Astrophysical Journal. Bd. 714 (1), 2010, S. 549–560, bibcode:2010ApJ...714..549H, doi:10.1088/0004-637X/714/1/549, arxiv:1003.3694.
- ↑ Sean M. Carroll: Interpreting Epsilon Aurigae. In: The Astrophysical Journal. Bd. 367, 1991, S 278–287, bibcode:1991ApJ...367..278C, doi:10.1086/169626.
- ↑ E. F. Guinan: Large distance of ε Aurigae inferred from interstellar absorption and reddening. In: Astronomy & Astrophysics. Bd. 546, 2012, Artikel-ID A123, bibcode:2012A&A...546A.123G, doi:10.1051/0004-6361/201118567.
- ↑ Z. Cvetković, B. Novaković: Orbits For Sixteen Binaries. In: Serbian Astronomical Journal. Bd. 173, 2006, S. 73–82, bibcode:2006SerAJ.173...73C, doi:10.2298/SAJ0673073C.
- ↑ Martin Adrian Barstow et al.: Resolving Sirius-like binaries with the Hubble Space Telescope. In: Monthly Notices of the Royal Astronomical Society. Bd. 322 (4), 2001, S. 891–900, bibcode:2001MNRAS.322..891B, doi:10.1046/j.1365-8711.2001.04203.x, arxiv:astro-ph/0010645.
- ↑ a b c d e f g Jay B. Holberg et al.: Where are all the Sirius-like binary systems? In: Monthly Notices of the Royal Astronomical Society. Bd. 435 (3), 2013, S. 2077–2091, bibcode:2013MNRAS.435.2077H, doi:10.1093/mnras/stt1433, arxiv:1307.8047.
- ↑ F. M. Rica Romero: Orbital Elements for BU 1240 AB. Nature of the C and D Components. In: Revista Mexicana de Astronomía y Astrofísica. Bd. 44, 2008, S. 137–147, bibcode:2008RMxAA..44..137R.
- ↑ R. K. Barry et al.: A Precise Physical Orbit for the M-dwarf Binary Gliese 268. In: The Astrophysical Journal. Bd. 760 (1), 2012, Artikel-ID 55, bibcode:2012ApJ...760...55B, doi:10.1088/0004-637X/760/1/55.
- ↑ a b c d J. Fernandes et al.: Fundamental stellar parameters for nearby visual binary stars: η Cas, ξ Boo, 70 Oph and 85 Peg. Helium abundance, age and mixing length parameter for low mass stars. In: Astronomy & Astrophysics, Bd. 338, 1998, S. 455–464, bibcode:1998A&A...338..455F.
- ↑ Francesco Borsa et al.: The GAPS programme with HARPS-N at TNG. VII. Putting exoplanets in the stellar context: magnetic activity and asteroseismology of τ Bootis A. In: Astronomy & Astrophysics. Bd. 578, 2015, Artikel-ID A64, bibcode:2015A&A...578A..64B, doi:10.1051/0004-6361/201525741, arxiv:1504.00491.
- ↑ Graham Hill et al.: Studies of late-type binaries. I – The physical parameters of 44ι Bootis ABC. In: Astronomy & Astrophysics. Bd. 211 (1), 1989, S. 81–98, bibcode:1989A&A...211...81H.
- ↑ Zackery W. Briesemeister et al.: High Spatial Resolution Thermal Infrared Spectroscopy with ALES: Resolved Spectra of the Benchmark Brown Dwarf Binary HD 130948BC. In: The Astronomical Journal. Bd. 157 (6), 2019, Artikel-ID 244, bibcode:2019AJ....157..244B, doi:10.3847/1538-3881/ab1901, arxiv:1904.07892.
- ↑ a b c Brian D. Mason et al.: Binary Star Orbits from Speckle Interferometry. I. Improved Orbital Elements of 22 Visual Systems. In: The Astronomical Journal. Bd. 117 (2), 1999, S. 1023–1036, bibcode:1999AJ....117.1023M, doi:10.1086/300748.
- ↑ Douglas S. Hall et al.: A Spectroscopic and Photometric Study of 12 BM Camelopardalis. In: The Astronomical Journal. Bd 109, 1995, S. 1277–1288, bibcode:1995AJ....109.1277H, doi:10.1086/117360.
- ↑ Kailash C. Sahu et al.: Relativistic deflection of background starlight measures the mass of a nearby white dwarf star. In: Science. Bd. 356 (6342), 2017, S. 1046–1050, bibcode:2017Sci...356.1046S, doi:10.1126/science.aal2879, arxiv:1706.02037.
- ↑ David S. Evans, Francis C. Fekel, Jr.: Beta Capricorni: fundamental parameters from occultation astrometry and spectroscopy. In: The Astrophysical Journal. Bd. 228, 1979, S. 497–508, bibcode:1979ApJ...228..497E, doi:10.1086/156872.
- ↑ Swetlana Hubrig et al.: New insights into the nature of the peculiar star θ Carinae. In: Astronomy & Astrophysics. Bd. 488 (1), 2008, S. 287–296, bibcode:2008A&A...488..287H, doi:10.1051/0004-6361:200809972, arxiv:0807.2067.
- ↑ a b c d e f Robert J. De Rosa et al.: The Volume-limited A-Star (VAST) survey – II. Orbital motion monitoring of A-type star multiples. In: Monthly Notices of the Royal Astronomical Society. Bd. 422 (4), 2012, S. 2765–2785, bibcode:2012MNRAS.422.2765D, doi:10.1111/j.1365-2966.2011.20397.x, arxiv:1112.3666.
- ↑ Myron A. Smith et al.: The relationship between γ Cassiopeiae’s X-ray emission and its circumstellar environment. In: Astronomy & Astrophysics. Bd. 540, 2012, Artikel-ID A53, bibcode:2012A&A...540A..53S, doi:10.1051/0004-6361/201118342, arxiv:1201.6415.
- ↑ a b c d e f g h Brian D. Mason et al.: The Washington Visual Double Star Catalog. VizieR-Datenkatalog B/wds (elektronisch veröffentlicht). 2021, bibcode:2021yCat....102026M.
- ↑ Julian C. Christou, Jack D. Drummond: Measurements of Binary Stars, Including Two New Discoveries, with the Lick Observatory Adaptive Optics System. In: The Astronomical Journal. Bd. 131 (6), 2006, S. 3100–3108, bibcode:2006AJ....131.3100C, doi:10.1086/503255.
- ↑ Jack D. Drummond et al.: ι Cassiopeiae: Orbit, Masses, and Photometry from Adaptive Optics Imaging in the I and H Bands. In: The Astrophysical Journal. Bd. 585 (2), 2003, S. 1007–1014, bibcode:2003ApJ...585.1007D, doi:10.1086/346224.
- ↑ Howard E. Bond et al.: Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age. In: The Astrophysical Journal. Bd. 904 (2), 2020, Arikel-ID 112, bibcode:2020ApJ...904..112B, doi:10.3847/1538-4357/abc172, arxiv:2010.06609.
- ↑ Robert J. De Rosa et al.: The VAST Survey – III. The multiplicity of A-type stars within 75 pc. In: Monthly Notices of the Royal Astronomical Society. Bd. 437 (2), 2014, S. 1216–1240, bibcode:2014MNRAS.437.1216D, doi:10.1093/mnras/stt1932, arxiv:1311.7141.
- ↑ David E. Holmgren et al.: Search for forced oscillations in binaries. III. Improved elements and the detection of line-profile variability of the B4V + A6V: system AR Cassiopeiae. In: Astronomy & Astrophysics. Bd. 345, 1999, S. 855–868, bibcode:1999A&A...345..855H.
- ↑ Pierre Kervella et al.: Proxima's orbit around α Centauri. In: Astronomy & Astrophysics. Bd. 598, 2017, Artikel-ID L7, bibcode:2017A&A...598L...7K, doi:10.1051/0004-6361/201629930, arxiv:1611.03495.
- ↑ Andrzej Pigulski et al.: Massive pulsating stars observed by BRITE-Constellation. I. The triple system β Centauri (Agena). In: Astronomy & Astrophysics. Bd. 588, 2016, Artikel-ID A55, bibcode:2016A&A...588A..55P, doi:10.1051/0004-6361/201527872, arxiv:1602.02806.
- ↑ a b c d Andrei A. Tokovinin: Speckle Interferometry and Orbits of "Fast" Visual Binaries. In: The Astronomical Journal. Bd. 144 (2), 2012, Artikel-ID 56, bibcode:2012AJ....144...56T, doi:10.1088/0004-6256/144/2/56, arxiv:1206.1882.
- ↑ E. Budding et al.: Absolute parameters of young stars – II. V831 Centauri. In: Monthly Notices of the Royal Astronomical Society. Bd. 403 (3), 2010, S. 1448–1456, bibcode:2010MNRAS.403.1448B, doi:10.1111/j.1365-2966.2010.16209.x.
- ↑ Hugh Wheelwright et al.: The close Be star companion of β Cephei. In: Astronomy & Astrophysics. Bd. 497 (2), 2009, S. 487–495, bibcode:2009A&A...497..487W, doi:10.1051/0004-6361/200811105, arxiv:0902.4356.
- ↑ Ralph Neuhäuser et al.: Direct detection of exoplanet host star companion γ Cep B and revised masses for both stars and the sub-stellar object. In: Astronomy & Astrophysics. Bd. 462 (2), 2007, S. 777–780, bibcode:2007A&A...462..777N, doi:10.1051/0004-6361:20066581, arxiv:astro-ph/0611427.
- ↑ George Gatewood et al.: Hipparcos and MAP Studies of the Triple Star π Cephei. In : The Astrophysical Journal. Bd. 549 (2), 2001, S. 1145–1150, bibcode:2001ApJ...549.1145G, doi:10.1086/319458.
- ↑ K. O. Wright: The System of VV Cephei Derived from an Analysis of the Hα Line. In: Journal of the Royal Astronomical Society of Canada. Bd. 71, 1977, S. 152–193, bibcode:1977JRASC..71..152W.
- ↑ L. Leedjärv et al.: The 1997/1998 eclipse of VV Cephei was late. In: Astronomy & Astrophysics. Bd. 349, 1999, S. 511–514, bibcode:1999A&A...349..511L.
- ↑ Wendy Hagen Bauer et al.: Spatial Extension in the Ultraviolet Spectrum of VV Cephei. In: The Astronomical Journal. Bd. 136 (3), 2008, S. 1312–1324, bibcode:2008AJ....136.1312H, doi:10.1088/0004-6256/136/3/1312.
- ↑ a b Xavier Delfosse et al.: Accurate masses of very low mass stars. IV. Improved mass-luminosity relations. In: Astronomy & Astrophysics. Bd. 364, 2000, S. 217–224, bibcode:2000A&A...364..217D, arxiv:astro-ph/0010586.
- ↑ S. P. Wyatt, J. H. Cahn: Kinematics and ages of Mira variables in the greater solar neighborhood. In: The Astrophysical Journal. Bd. 275, 1983, S. 225–239, bibcode:1983ApJ...275..225W, doi:10.1086/161527.
- ↑ a b G. Fritz Benedict et al.: The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs. In: The Astronomical Journal. Bd. 152 (5), 2016, Artikel-ID 141, bibcode:2016AJ....152..141B, doi:10.3847/0004-6256/152/5/141, arxiv:1608.04775.
- ↑ César Briceño, Andrei A. Tokovinin: New Binaries in the ɛ Cha Association. In: The Astronomical Journal. Bd. 154 (5), 2017, Artikel-ID 195, bibcode:2017AJ....154..195B, doi:10.3847/1538-3881/aa8e9b, arxiv:1709.05044.
- ↑ Howard E. Bond et al.: The Sirius System and Its Astrophysical Puzzles: Hubble Space Telescope and Ground-based Astrometry. In: The Astrophysical Journal. Bd. 840 (2), 2017, Artikel-ID 70, bibcode:2017ApJ...840...70B, doi:10.3847/1538-4357/aa6af8, arxiv:1703.10625.
- ↑ a b Jesús Maíz Apellániz, R. H. Barbá: Spatially resolved spectroscopy of close massive visual binaries with HST/STIS. I. Seven O-type systems. In: Astronomy & Astrophysics. Bd. 636, 2020, Artikel-ID A28, bibcode:2020A&A...636A..28M, doi:10.1051/0004-6361/202037730, arxiv:2002.12149.
- ↑ William G. Bagnuolo, Jr. et al.: Tomographic Separation of Composite Spectra. II. The Components of 29 UW Canis Majoris. In: The Astrophysical Journal. Bd. 423, 1994, S. 446–455, bibcode:1994ApJ...423..446B, doi:10.1086/173822.
- ↑ James Liebert et al.: The Age and Stellar Parameters of the Procyon Binary System. In: The Astrophysical Journal. Bd. 769 (1), 2013, Artikel-ID 7, bibcode:2013ApJ...769....7L, doi:10.1088/0004-637X/769/1/7, arxiv:1305.0587.
- ↑ J. B. Hutchings et al.: Direct Observation of the Fourth Star in the ζ Cancri System. In: Publications of the Astronomical Society of the Pacific. Bd. 112 (772), 2000, S. 833–836, bibcode:2000PASP..112..833H, doi:10.1086/316587, arxiv:astro-ph/0004284.
- ↑ Adam J. Burgasser et al.: Multiplicity among Widely Separated Brown Dwarf Companions to Nearby Stars: Gliese 337CD. In: The Astronomical Journal. Bd. 129 (6), 2005, S. 2849–2855, bibcode:2005AJ....129.2849B, doi:10.1086/430218, arxiv:astro-ph/0503379.
- ↑ Roxanne Ligi et al.: Radii, masses, and ages of 18 bright stars using interferometry and new estimations of exoplanetary parameters. In: Astronomy & Astrophysics. Bd. 586, 2016, Artikel-ID A94, bibcode:2016A&A...586A..94L, doi:10.1051/0004-6361/201527054, {{arXiv:1511.03197}}.
- ↑ a b Elisabeth R. Newton et al.: The Hα Emission of Nearby M Dwarfs and its Relation to Stellar Rotation. In: The Astrophysical Journal. Bd. 834 (1), 2017, Artikel-ID 85, bibcode:2017ApJ...834...85N, doi:10.3847/1538-4357/834/1/85, arxiv:1611.03509.
- ↑ a b Maciej Konacki et al.: High-precision Orbital and Physical Parameters of Double-lined Spectroscopic Binary Stars – HD78418, HD123999, HD160922, HD200077, and HD210027. In: The Astrophysical Journal. Bd. 719 (2), 2010, S. 1293–1314, bibcode:2010ApJ...719.1293K, doi:10.1088/0004-637X/719/2/1293, arxiv:0910.4482.
- ↑ Gijs H. A. Roelofs et al.: Spectroscopic Evidence for a 5.4 Minute Orbital Period in HM Cancri. In: The Astrophysical Journal Letters. Bd. 711 (2), 2010, L138–L142, bibcode:2010ApJ...711L.138R, doi:10.1088/2041-8205/711/2/L138, arxiv:1003.0658.
- ↑ a b N. Todorović, R. Pavlović: Orbits of Seven Edge-On Visual Double Stars. In: Serbian Astronomical Journal. Bd. 170, 2005, S. 73–78, bibcode:2005SerAJ.170...73P, doi:10.2298/SAJ0570073P.
- ↑ John M. Brewer et al.: Spectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars. In: The Astrophysical Journal Supplement Series. Bd. 225 (2), 2016, Artikel-ID 32, bibcode:2016ApJS..225...32B, doi:10.3847/0067-0049/225/2/32, arxiv:1606.07929.
- ↑ J. Tomkin, D. M. Popper: Rediscussion of eclipsing binarties. XV. Alpha Coronae Borealis, a main-sequence system with components of types A and G. In: The Astronomical Journal. Bd. 91, 1986, S. 1428–1437, bibcode:1986AJ.....91.1428T, doi:10.1086/114121.
- ↑ Hans Bruntt et al.: The radius and effective temperature of the binary Ap star β CrB from CHARA/FLUOR and VLT/NACO observations. In: Astronomy & Astrophysics. Bd. 512, 2010, Artikel-ID A55, bibcode:2010A&A...512A..55B, doi:10.1051/0004-6361/200913405, arxiv:0912.3215.
- ↑ Deepak Raghavan et al.: The Visual Orbit of the 1.1 Day Spectroscopic Binary σ2 Coronae Borealis from Interferometry at the Chara Array. In: The Astrophysical Journal. Bd. 690 (1), 2009, S. 394–406, bibcode:2009ApJ...690..394R, doi:10.1088/0004-637X/690/1/394, arxiv:0808.4015.
- ↑ Carlos A. Hernández, Elida B. de Hernández: The orbital elements of 25 G CRU (HD 108250). In: Revista Mexicana de Astronomía y Astrofísica. Bd. 4, 1979, S. 297–300, bibcode:1979RMxAA...4..297H.
- ↑ Francis C. Fekel et al.: Absolute Properties of the Eclipsing Binary VV Corvi. In: The Astronomical Journal. Bd. 146 (6), 2013, Artikel-ID 146, bibcode:2013AJ....146..146F, doi:10.1088/0004-6256/146/6/146.
- ↑ Zeki Eker, L. R. Doherty: Hα region spectroscopy of the RS CVn system HR 5110. In: Monthly Notices of the Royal Astronomical Society. Bd. 228, 1987, S. 869–881, bibcode:1987MNRAS.228..869E, doi:10.1093/mnras/228.4.869.
- ↑ Ronald Drimmel et al.: A celestial matryoshka: dynamical and spectroscopic analysis of the Albireo system. In: Monthly Notices of the Royal Astronomical Society. Bd. 502 (1), 2021, S. 328–350, bibcode:2021MNRAS.502..328D, doi:10.1093/mnras/staa4038, arxiv:2012.01277.
- ↑ Fang Xia, Yanning Fu: The Dynamical State and Long-term Stability of HIP 102589. In: The Astrophysical Journal. Bd. 814 (1), 2015, Artikel-ID 64, bibcode:2015ApJ...814...64X, doi:10.1088/0004-637X/814/1/64.
- ↑ a b Joel A. Eaton et al.: Orbits and Pulsations of the Classical ζ Aurigae Binaries. In: The Astrophysical Journal. Bd. 679 (2), 2008, S. 1490–1498, bibcode:2008ApJ...679.1490E, doi:10.1086/587452, arxiv:0802.2238.
- ↑ Francis C. Fekel: The Spectroscopic Orbit of φ Cygni, a System with Two Late-Type Giants. In: Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). Bd. 21, 2004, S. 63–64, bibcode:2004RMxAC..21...63F.
- ↑ Heather M. Hauser, Geoffrey W. Marcy: The Orbit of 16 Cygni AB. In: Publications of the Astronomical Society of the Pacific. Bd. 111 (757), 1999, S. 321–334, bibcode:1999PASP..111..321H, doi:10.1086/316328.
- ↑ Marcelo Tucci Maia et al.: Revisiting the 16 Cygni planet host at unprecedented precision and exploring automated tools for precise abundances. In: Astronomy & Astrophysics. Bd. 628, 2019, Artikel-ID A126, bibcode:2019A&A...628A.126M, doi:10.1051/0004-6361/201935952, arxiv:1906.04195.
- ↑ Pierre Kervella et al.: The radii of the nearby K5V and K7V stars 61 Cygni A & B. CHARA/FLUOR interferometry and CESAM2k modeling. In: Astronomy & Astrophysics. Bd. 488 (2), 2008, S. 667–674, bibcode:2008A&A...488..667K, doi:10.1051/0004-6361:200810080, arxiv:0806.4049.
- ↑ Nicholas Law et al.: The LuckyCam survey for very low mass binaries – II. 13 new M4.5-M6.0 binaries. In: Monthly Notices of the Royal Astronomical Society. Bd. 384 (1), 2008, S. 150–160, bibcode:2008MNRAS.384..150L, doi:10.1111/j.1365-2966.2007.12675.x, arxiv:0704.1812.
- ↑ a b Tyler Gardner et al.: ARMADA. I. Triple Companions Detected in B-type Binaries α Del and ν Gem. In: The Astronomical Journal. Bd. 161 (1), 2021, Artikel-ID 40, bibcode:2021AJ....161...40G, doi:10.3847/1538-3881/abcf4e, arxiv:2012.00778.
- ↑ a b James W. Davidson, Jr. et al.: A Photometric Analysis of Seventeen Binary Stars Using Speckle Imaging. In: The Astronomical Journal. Bd. 138 (5), 2009, S. 1354–1364, bibcode:2009AJ....138.1354D; doi:10.1088/0004-6256/138/5/1354.
- ↑ Tyler Gardner et al.: Precision Orbit of δ Delphini and Prospects for Astrometric Detection of Exoplanets. In: The Astrophysical Journal. Bd. 855 (1),2018, Artikel-ID 1, bibcode:2018ApJ...855....1G, doi:10.3847/1538-4357/aaac80, arxiv:1802.00468.
- ↑ Jiří Kubát et al.: Spectroscopy of close visual binary components of the stable shell star 1 Delphini. In: Astronomy & Astrophysics. Bd. 587, 2016, Artikel-ID A22, bibcode:2016A&A...587A..22K, doi:10.1051/0004-6361/201526414, arxiv:1601.05236.
- ↑ Einzelhelligkeiten aus scheinbarer Gesamthelligkeit V = 3,65 mag (Bright Star Catalogue) und Helligkeitsdifferenz ΔmV = 1,8 (Don Hutter et al.: Surveying the Bright Stars by Optical Interferometry. I. A Search for Multiplicity among Stars of Spectral Types F-K. In: The Astrophysical Journal Supplement Series. Bd. 227 (1), 2016, Artikel-ID 4, bibcode:2016ApJS..227....4H, doi:10.3847/0067-0049/227/1/4, arxiv:1609.05254) berechnet.
- ↑ a b Bradford B. Behr et al.: Stellar Astrophysics with a Dispersed Fourier Transform Spectrograph. I. Instrument Description and Orbits of Single-lined Spectroscopic Binaries. In: The Astrophysical Journal. Bd. 705 (1), 2009, S. 543–553, bibcode:2009ApJ...705..543B, doi:10.1088/0004-637X/705/1/543, arxiv:0909.3241.
- ↑ a b c C. Martin et al.: Mass determination of astrometric binaries with Hipparcos. III. New results for 28 systems. In: Astronomy & Astrophysics Supplement. Bd. 133, 1998, S. 149–162, bibcode:1998A&AS..133..149M, doi:10.1051/aas:1998459.
- ↑ Rachael M. Roettenbacher et al.: Detecting the Companions and Ellipsoidal Variations of RS CVn Primaries. II. o Draconis, a Candidate for Recent Low-mass Companion Ingestion. In: The Astrophysical Journal. Bd. 809 (2), 2015, Artikel-ID 159, bibcode:2015ApJ...809..159R, doi:10.1088/0004-637X/809/2/159, arxiv:1507.03601.
- ↑ Andrei A. Tokovinin et al.: Fundamental parameters and origin of the very eccentric binary 41 Dra. In: Astronomy & Astrophysics. Bd. 409, 2003, S. 245–250, bibcode:2003A&A...409..245T, doi:10.1051/0004-6361:20031064.
- ↑ a b c Pierre Kervella et al.: Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly. In: Astronomy & Astrophysics. Bd. 623, 2019, Artikel-ID A72, bibcode:2019A&A...623A..72K, doi:10.1051/0004-6361/201834371, arxiv:1811.08902.
- ↑ Beate Stelzer et al.: Search of X-ray emission from roAp stars: the case of γ Equulei. In: Astronomy & Astrophysics. Bd. 529, 2011, Artikel-ID A29, bibcode:2011A&A...529A..29S, doi:10.1051/0004-6361/201016265, arxiv:1103.0739.
- ↑ Birgitta Nordström et al.: Geneva-Copenhagen Survey of Solar neighbourhood. VizieR-Datenkatalog V/117A (elektronisch veröffentlicht). 2008, bibcode:2008yCat.5117....0N.
- ↑ Brian D. Mason et al.: Binary Star Orbits. V. The Nearby White Dwarf/Red Dwarf Pair 40 Eri BC. In: The Astronomical Journal. Bd. 154 (5), 2017, Artikel-ID 200, bibcode:2017AJ....154..200M, doi:10.3847/1538-3881/aa803e, arxiv:1707.03635.
- ↑ Daryl W. Willmarth et al.: Spectroscopic Orbits for 15 Late-type Stars. In: The Astronomical Journal. Bd. 152 (2), 2016, Artikel-ID 46, doi:10.3847/0004-6256/152/2/46, bibcode:2016AJ....152...46W.
- ↑ Andrei A. Tokovinin: Kappa Fornaci, A Triple Radio Star. In: The Astronomical Journal. Bd. 145 (3), 2013, Artikel-ID 76, bibcode:2013AJ....145...76T, doi:10.1088/0004-6256/145/3/76, arxiv:1301.1352.
- ↑ Manuel Andrade, José A. Docobo: The Dynamical Evolution of the Multiple Stellar System α Gem. In: Living Together: Planets, Host Stars and Binaries. ASP Conference Series, Astronomical Society of the Pacific, Bd. 496, 2015, S. 94–98, bibcode:2015ASPC..496...94A.
- ↑ Aurore Blazère et al.: Discovery of a very weak magnetic field on the Am star Alhena. In: Monthly Notices of the Royal Astronomical Society: Letters. Bd. 459 (1), 2016, L81–L84, bibcode:2016MNRAS.459L..81B, doi:10.1093/mnrasl/slw050, arxiv:1603.06486.
- ↑ Benjamin F. Lane et al.: The Orbits of the Triple-star System 1 Geminorum from Phases Differential Astrometry and Spectroscopy. In: The Astrophysical Journal. Bd. 783 (1), 2014, Artikel-ID 3, bibcode:2014ApJ...783....3L, doi:10.1088/0004-637X/783/1/3.
- ↑ Samantha C. Searle et al.: Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters. In: Astronomy & Astrophysics. Bd. 481 (3), 2008, S. 777–797, bibcode:2008A&A...481..777S, doi:10.1051/0004-6361:20077125, arxiv:0801.4289.
- ↑ a b Matthew W. Muterspaugh et al.: The Phases Differential Astrometry Data Archive. IV. The Triple Star Systems 63 Gem A and HR 2896. In: The Astronomical Journal. Bd. 140 (6), 2010, S. 1646–1656, bibcode:2010AJ....140.1646M, doi:10.1088/0004-6256/140/6/1646, arxiv:1010.4045.
- ↑ Ehsan Moravveji et al.: The age and mass of the α Herculis triple-star system from a MESA grid of rotating stars with 1.3 ≤ M/M☉ ≤ 8.0. In: The Astronomical Journal. Bd. 146 (3), 2013, Artikel-ID 148, bibcode:2013AJ....146..148M, doi:10.1088/0004-6256/146/6/148, arxiv:1308.1632.
- ↑ Xiaopei P. Pan et al.: The Visual Orbit, the Stellar Diameter and the Magnitude Difference of the Spectroscopic Binary β Herculis. In: Bulletin of the American Astronomical Society. Bd. 22, 1990, S. 1335, bibcode:1990BAAS...22R1335P.
- ↑ Pierre Morel et al.: The ζ Herculis binary system revisited. Calibration and seismology. In: Astronomy & Astrophysics. Bd. 379, 2001, S. 245–256, bibcode:2001A&A...379..245M, doi:10.1051/0004-6361:20011336, arxiv:astro-ph/0110004.
- ↑ Lewis C. Roberts, Jr. et al.: Characterization of the Companion μ Her. In: The Astronomical Journal. Bd. 151 (6), 2016, Artikel-ID 169, bibcode:2016AJ....151..169R, doi:10.3847/0004-6256/151/6/169, arxiv:1604.06494.
- ↑ J.-L. Prieur et al.: Speckle observations with PISCO in Merate: XIII. Astrometric measurements of visual binaries in 2012, and new orbits for ADS 10786 BC, 12144, 12515, 16314 and 16539. In: Astronomische Nachrichten. Bd. 335 (8), 2014, S. 817 ff., bibcode:2014AN....335..817P, doi:10.1002/asna.201412054.
- ↑ Guillermo Torres: Astrometric-Spectroscopic Determination of the Absolute Masses of the HgMn Binary Star φ Herculis. In: The Astronomical Journal. Bd. 133 (6), 2007, S. 2684–2695, bibcode:2007AJ....133.2684T, doi:10.1086/516756, arxiv:astro-ph/0703193.
- ↑ James Sikora et al.: A volume-limited survey of mCP stars within 100 pc – I. Fundamental parameters and chemical abundances. In: Monthly Notices of the Royal Astronomical Society. Bd. 483 (2), 2019, S. 2300–2324, bibcode:2019MNRAS.483.2300S, doi:10.1093/mnras/sty3105, arxiv:1811.05633.
- ↑ Grant M. Kennedy et al.: 99 Herculis: host to a circumbinary polar-ring debris disc. In: Monthly Notices of the Royal Astronomical Society. Bd. 421 (3), 2012, S. 2264–2276, bibcode:2012MNRAS.421.2264K, doi:10.1111/j.1365-2966.2012.20448.x, arxiv:1201.1911.
- ↑ a b Matthew W. Muterspaugh et al.: Masses, Luminosities, and Orbital Coplanarities of the μ Orionis Quadruple-Star System from Phases Differential Astrometry. In: The Astronomical Journal. Bd. 135 (3), 2008, S. 766–776, bibcode:2008AJ....135..766M, doi:10.1088/0004-6256/135/3/766, arxiv:0710.2126.
- ↑ E. Zhang et al.: The 71 Second Oscillation in the Light Curve of the Old Nova DQ Herculis. In: The Astrophysical Journal. Bd. 454, 1995, S. 447–462, bibcode:1995ApJ...454..447Z, doi:10.1086/176496.
- ↑ a b c Lindsay Marion et al.: Searching for faint companions with VLTI/PIONIER. II. 92 main sequence stars from the Exozodi survey. In: Astronomy & Astrophysics. Bd. 570, 2014, Artikel-ID A127, bibcode:2014A&A...570A.127M, doi:10.1051/0004-6361/201424780, arxiv:1409.6105.
- ↑ Brice-Olivier Demory et al.: Mass-radius relation of low and very low-mass stars revisited with the VLTI. In Astronomy & Astrophysics. Bd. 505 (1), 2009, S. 205–215, bibcode:2009A&A...505..205D, doi:10.1051/0004-6361/200911976, arxiv:0906.0602.
- ↑ Robert King et al.: ɛ Indi Ba, Bb: a detailed study of the nearest known brown dwarfs. In: Astronomy & Astrophysics. Bd. 510, 2010, Artikel-ID A99, bibcode:2010A&A...510A..99K, doi:10.1051/0004-6361/200912981, arxiv:0911.3143.
- ↑ Douglas R. Gies et al.: A Spectroscopic Orbit for Regulus. In: The Astrophysical Journal Letters. Bd. 682 (2), 2008, L117–L120, bibcode:2008ApJ...682L.117G, doi:10.1086/591148, arxiv:0806.3473.
- ↑ Douglas R. Gies et al.: Spectroscopic Detection of the Pre-White Dwarf Companion of Regulus. In: The Astrophysical Journal. Bd. 902 (1), 2020, Artikel-ID 25, bibcode:2020ApJ...902...25G, doi:10.3847/1538-4357/abb372, arxiv:2009.02409.
- ↑ Saul Rappaport et al.: The Past and Future History of Regulus. In: The Astrophysical Journal. Bd. 698 (1), 2009, S. 666–675, bibcode:2009ApJ...698..666R, doi:10.1088/0004-637X/698/1/666, arxiv:0904.0395.
- ↑ S.-L. Bi et al.: Seismological Analysis of the Stars γ Serpentis and ι Leonis: Stellar Parameters and Evolution. In: The Astrophysical Journal. Bd. 673 (2), 2008, S. 1093–1105, bibcode:2008ApJ...673.1093B, doi:10.1086/521575.
- ↑ R. E. M. Griffin, R. F. Griffin: Composite spectra Paper 13: 93 Leonis, a chromospherically-active binary. In: Monthly Notices of the Royal Astronomical Society. Bd. 350 (2), 2004, S. 685–706, bibcode:2004MNRAS.350..685G, doi:10.1111/j.1365-2966.2004.07680.x.
- ↑ Tadashi Nakajima et al.: Physical Properties of Gliese 229B Based on Newly Determined Carbon and Oxygen Abundances of Gliese 229A. In: The Astronomical Journal. Bd. 150 (2), 2015, Artikel-ID 53, bibcode:2015AJ....150...53N, doi:10.1088/0004-6256/150/2/53, arxiv:1506.03178 .
- ↑ José A. Caballero: Reaching the boundary between stellar kinematic groups and very wide binaries . II. α Librae + KU Librae: a common proper motion system in Castor separated by 1.0 pc. In: Astronomy & Astrophysics. Bd. 514, 2010, Artikel-ID A98, bibcode:2010A&A...514A..98C, doi:10.1051/0004-6361/200913986, arxiv:1001.5432.
- ↑ Klaus Fuhrmann et al.: On the bright A-type star Alpha Librae A. In: Monthly Notices of the Royal Astronomical Society. Bd. 437 (3), 2014, S. 2303–2306, bibcode:2014MNRAS.437.2303F, doi:10.1093/mnras/stt2046.
- ↑ Michael R. Line et al.: Uniform Atmospheric Retrieval Analysis of Ultracool Dwarfs. I. Characterizing Benchmarks, Gl 570D and HD 3651B. In: The Astrophysical Journal. Bd. 807 (2), 2015, Artikel-ID 183, bibcode:2015ApJ...807..183L, doi:10.1088/0004-637X/807/2/183, arxiv:1504.06670.
- ↑ a b Siegfried Eggl et al.: Circumstellar habitable zones of binary-star systems in the solar neighbourhood. In: Monthly Notices of the Royal Astronomical Society. Bd. 428 (4), 2013, S. 3104–3113, bibcode:2013MNRAS.428.3104E, doi:10.1093/mnras/sts257, arxiv:1210.5411.
- ↑ Ming Zhao et al.: First Resolved Images of the Eclipsing and Interacting Binary β Lyrae. In: The Astrophysical Journal Letters. Bd. 684 (2), 2008, L95–L98, bibcode:2008ApJ...684L..95Z, doi:10.1086/592146, arxiv:0808.0932.
- ↑ Andrei A. Tokovinin: Comparative statistics and origin of triple and quadruple stars. In: Monthly Notices of the Royal Astronomical Society. Bd. 389 (2), 2008, S. 925–938, bibcode:2008MNRAS.389..925T, doi:10.1111/j.1365-2966.2008.13613.x, arxiv:0806.3263.
- ↑ Ricky Nilsson et al.: Project 1640 Observations of Brown Dwarf GJ 758 B: Near-infrared Spectrum and Atmospheric Modeling. In: The Astrophysical Journal. Bd. 838 (1), 2017, Artikel-ID 64, bibcode:2017ApJ...838...64N, doi:10.3847/1538-4357/aa643c, arxiv:1703.01023.
- ↑ Ján Budaj, Ilian Kh. Iliev: Abundance analysis of Am binaries and search for tidally driven abundance anomalies – I. HD 33254, HD 178449 and HD 198391. In: Monthly Notices of the Royal Astronomical Society. Bd. 346 (1), 2003, S. 27–36, bibcode:2003MNRAS.346...27B, doi:10.1046/j.1365-2966.2003.07071.x.
- ↑ Jesús Maíz Apellániz: Gaia DR2 distances to Collinder 419 and NGC 2264 and new astrometric orbits for HD 193 322 Aa,Ab and 15 Mon Aa,Ab. In: Astronomy & Astrophysics. Bd. 630, 2019, Artikel-ID A119, bibcode:2019A&A...630A.119M, doi:10.1051/0004-6361/201935885, arxiv:1908.02040.
- ↑ Don R. Chance, John L. Hershey: Separate Spectra of the Components of the Low-Mass Binaries Ross 614A,B and L722-22A,B. In: Publications of the Astronomical Society of the Pacific. Bd. 110 (746), 1998, S. 425–432, bibcode:1998PASP..110..425C, doi:10.1086/316146.
- ↑ George Gatewood et al.: An Astrometric Study of the Low-Mass Binary Star Ross 614. In: The Astronomical Journal. Bd. 125 (3), 2003, S. 1530–1536, bibcode:2003AJ....125.1530G, doi:10.1086/346143.
- ↑ Eric E. Mamajek et al.: The Closest Known Flyby of a Star to the Solar System. In: The Astrophysical Journal Letters. Bd. 800 (1), 2015, Artikel-ID L17, bibcode:2015ApJ...800L..17M, doi:10.1088/2041-8205/800/1/L17, arxiv:1502.04655.
- ↑ Trent J. Dupuy et al.: WISE J072003.20-084651.2B is a Massive T Dwarf. In: The Astronomical Journal. Bd. 158 (5), 2019, Artikel-ID 174, bibcode:2019AJ....158..174D, doi:10.3847/1538-3881/ab3cd1, arxiv:1908.06994.
- ↑ Yasuharu Sugawara et al.: Redshifted emission lines and radiative recombination continuum from the Wolf-Rayet binary θ Muscae: evidence for a triplet system? In: Astronomy & Astrophysics. Bd. 490 (1), 2008, S. 259–264, bibcode:2008A&A...490..259S, doi:10.1051/0004-6361:20079302, arxiv:0810.1208.
- ↑ A. D. Thackeray: Orbits of two double-lined spectroscopic binaries HD 147971 and 75759. In: Monthly Notices of the Royal Astronomical Society. Bd. 134, 1966, S. 97–106, bibcode:1966MNRAS.134...97T, doi:10.1093/mnras/134.1.97.
- ↑ Sasha Hinkley et al.: Establishing α Oph as a Prototype Rotator: Improved Astrometric Orbit. In: The Astrophysical Journal. Bd. 726 (2), 2011, Artikel-ID 104, bibcode:2011ApJ...726..104H, doi:10.1088/0004-637X/726/2/104, arxiv:1010.4028.
- ↑ José A. Docobo, J. F. Ling: Orbits and System Masses of 14 Visual Double Stars with Early-Type Components. In: The Astronomical Journal. Bd. 133 (4), 2007, S. 1209–1216, bibcode:2007AJ....133.1209D, doi:10.1086/511070.
- ↑ Alan W. Irwin et al.: 36 Ophiuchi AB: Incompatibility of the Orbit and Precise Radial Velocities. In: Publications of the Astronomical Society of the Pacific. Bd. 108, 1996, S. 580–590, bibcode:1996PASP..108..580I, doi:10.1086/133768.
- ↑ Xiaoli Wang et al.: The Three-dimensional Orbit and Physical Parameters of 47 Oph. In: The Astronomical Journal. Bd. 149 (3), 2015, Artikel-ID 110, bibcode:2015AJ....149..110W, doi:10.1088/0004-6256/149/3/110.
- ↑ Tsevi Mazeh et al.: Studies of multiple stellar systems – IV. The triple-lined spectroscopic system Gliese 644. In: Monthly Notices of the Royal Astronomical Society. Bd. 325 (1), 2001, S. 343–357, bibcode:2001MNRAS.325..343M, doi:10.1046/j.1365-8711.2001.04419.x, arxiv:astro-ph/0102451.
- ↑ Joanna Mikołajewska, Michael M. Shara: The Massive CO White Dwarf in the Symbiotic Recurrent Nova RS Ophiuchi. In: The Astrophysical Journal. Bd. 847 (2), 2017, Artikel-ID 99, bibcode:2017ApJ...847...99M, doi:10.3847/1538-4357/aa87b6, arxiv:1702.08732.
- ↑ Tomer Shenar et al.: A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis. In: The Astrophysical Journal. Bd. 809 (2), 2015, Artikel-ID 135, bibcode:2015ApJ...809..135S, doi:10.1088/0004-637X/809/2/135, arxiv:1503.03476.
- ↑ Christian A. Hummel et al.: Dynamical mass of the O-type supergiant in ζ Orionis A. In: Astronomy & Astrophysics. Bd. 554, 2013, Artikel-ID A52, bibcode:2013A&A...554A..52H, doi:10.1051/0004-6361/201321434, arxiv:1306.0330.
- ↑ a b c d GRAVITY Collaboration (Martina Karl et al.): Multiple star systems in the Orion nebula. In: Astronomy & Astrophysics. Bd. 620, 2018, Artikel-ID A116, bibcode:2018A&A...620A.116G, doi:10.1051/0004-6361/201833575, arxiv:1809.10376.
- ↑ a b c d Stefan Kraus et al.: Tracing the young massive high-eccentricity binary system θ1 Orionis C through periastron passage. In: Astronomy & Astrophysics. Bd. 497 (1), 2009, S. 195–207, bibcode:2009A&A...497..195K, doi:10.1051/0004-6361/200810368, arxiv:0902.0365.
- ↑ Yu. Yu. Balega et al.: Young massive binary θ1 Ori C: Radial velocities of components. In: Astrophysical Bulletin. Bd. 69 (1), 2014, S. 46–57, bibcode:2014AstBu..69...46B, doi:10.1134/S1990341314010052.
- ↑ Herbert Pablo et al.: The most massive heartbeat: an in-depth analysis of ι Orionis. In: Monthly Notices of the Royal Astronomical Society. Bd. 467 (2), 2017, S. 2494–2503, bibcode:2017MNRAS.467.2494P, doi:10.1093/mnras/stx207, arxiv:1703.02086.
- ↑ Gail Schaefer et al.: Orbits, Distance, and Stellar Masses of the Massive Triple Star σ Orionis. In: The Astronomical Journal. Bd. 152 (6), 2016, Artikel-ID 213, bibcode:2016AJ....152..213S, doi:10.3847/0004-6256/152/6/213, arxiv:1610.01984.
- ↑ B. König et al.: Direct detection of the companion of χ1 Orionis. In: Astronomy & Astrophysics. Bd. 394, 2002, S. L43–L46, doi:10.1051/0004-6361:20021377, arxiv:astro-ph/0209404, bibcode:2002A&A...394L..43K.
- ↑ Jinyoung Serena Kim et al.: Proplyds Around a B1 Star: 42 Orionis in NGC 1977. In: The Astrophysical Journal Letters. Bd. 826 (1), 2016, Artikel-ID L15, bibcode:2016ApJ...826L..15K, doi:10.3847/2041-8205/826/1/L15, arxiv:1606.08271.
- ↑ C. D. Scarfe et al.: 64 Orionis: Three-Dimensional Orbit and Physical Parameters. In: The Astronomical Journal. Bd. 119 (5), 2000, S. 2415–2421, bibcode:2000AJ....119.2415S, doi:10.1086/301366.
- ↑ J . Andersen et al.: Absolute dimensions of eclipsing binaries. XVI. V1031 Orionis In: Astronomy & Astrophysics. Bd. 228, 1990, S. 365–378, bibcode:1990A&A...228..365A.
- ↑ Markus Kasper et al.: The very nearby M/T dwarf binary SCR 1845-6357. In: Astronomy & Astrophysics. Bd. 471 (2), 2007, S. 655–659, bibcode:2007A&A...471..655K, doi:10.1051/0004-6361:20077881, arxiv:0706.3824.
- ↑ Christian A. Hummel et al.: Navy Prototype Optical Interferometer Observations of the Double Stars Mizar A and Matar. In: The Astronomical Journal. Bd. 116 (5), 1998, S. 2536–2548. bibcode:1998AJ....116.2536H, doi:10.1086/300602.
- ↑ Matthew W. Muterspaugh et al.: PHASES Differential Astrometry and Iodine Cell Radial Velocities of the κ Pegasi Triple Star System. In: The Astrophysical Journal. Bd. 636 (2), 2006, S. 1020–1032, bibcode:2006ApJ...636.1020M, doi:10.1086/498209, arxiv:astro-ph/0509406.
- ↑ Andrei A. Tokovinin: Inner and Outer Orbits in 13 Resolved Hierarchical Stellar Systems. In: Astronomical Journal. Bd. 161 (3), 2021, Artikel-ID 144, bibcode:2021AJ....161..144T, doi:10.3847/1538-3881/abda42, arxiv:2101.02976.
- ↑ Alain Jorissen et al.: Barium and related stars, and their white-dwarf companions. I. Giant stars. In: Astronomy & Astrophysics. Bd. 626, 2019, Artikel-ID A127, bibcode:2019A&A...626A.127J, doi:10.1051/0004-6361/201834630, arxiv:1904.03975.
- ↑ Fabien Baron et al.: Imaging the Algol Triple System in the H Band with the CHARA Interferometer. In: The Astrophysical Journal. Bd. 752 (1), 2012, Artikel-ID 20, bibcode:2012ApJ...752...20B, doi:10.1088/0004-637X/752/1/20, arxiv:1205.0754.
- ↑ Jiri Libich et al.: The new orbital elements and properties of ε Persei. In: Astronomy & Astrophysics. Bd. 446 (2), 2006, S. 583–589, bibcode:2006A&A...446..583L, doi:10.1051/0004-6361:20053032.
- ↑ D. J. Stickland, C. Lloyd: Spectroscopic binary orbits from ultraviolet radial velocities. Paper 28: ο Persei. In: The Observatory. Bd. 118, 1998, S 138–144, bibcode:1998Obs...118..138S.
- ↑ L. S. Lyubimkov et al.: The binary system o Per: Orbital elements, component parameters, and helium abundance. In: Astronomy Reports. Bd. 41 (5), 1997, S. 630–638, bibcode:1997ARep...41..630L.
- ↑ William Foster van Altena et al.: Yale Trigonometric Parallaxes, Fourth Edition. VizieR-Datenkatalog I/238A (elektronisch veröffentlicht). 2001, bibcode:2001yCat.1238....0V.
- ↑ Eric E. Mamajek et al.: The Solar Neighborhood. XXX. Fomalhaut C. In: The Astronomical Journal. Bd. 146 (6), 2013, Artikel-ID 154, bibcode:2013AJ....146..154M, doi:10.1088/0004-6256/146/6/154, arxiv:1310.0764.
- ↑ Dimitri Pourbaix, H. M. J. Boffin: Reprocessing the Hipparcos Intermediate Astrometric Data of spectroscopic binaries. II. Systems with a giant component. In: Astronomy & Astrophysics. Bd. 398, 2003, S. 1163–1177, bibcode:2003A&A...398.1163P, doi:10.1051/0004-6361:20021736, arxiv:astro-ph/0211483.
- ↑ Gilles Duvert et al.: Phase closure nulling of HD 59717 with AMBER/VLTI . Detection of the close faint companion. In: Astronomy & Astrophysics. Bd. 509, 2010, Artikel-ID A66, bibcode:2010A&A...509A..66D, doi:10.1051/0004-6361/200811037, arxiv:1001.5010.
- ↑ L. P. R. Vaz, J. Andersen: Absolute dimensions of eclipsing binaries. IV. PV Puppis, a detached late A-type system with equal, intrinsically variable components. In: Astronomy & Astrophysics. Bd. 132, 1984, S. 219–228, bibcode:1984A&A...132..219V.
- ↑ Andrei Tokovinin et al.: Speckle Interferometry at SOAR in 2014. In: The Astronomical Journal. Bd. 150 (2), 2015, Artikel-ID 50, bibcode:2015AJ....150...50T, doi:10.1088/0004-6256/150/2/50, arxiv:1506.05718.
- ↑ Genya Takeda et al.: Stellar parameters of nearby cool stars. VizieR-Datenkatalog J/ApJS/168/297 (elektronisch veröffentlicht). 2008, bibcode:2008yCat..21680297T.
- ↑ Mounib F. El Eid: CNO isotopes in red giants: theory versus observations. In: Astronomy & Astrophysics. Bd. 285, 1994, S. 915–928, bibcode:1994A&A...285..915E.
- ↑ R. P. Kudritzki, D. Reimers: On the absolute scale of mass-loss in red giants. II. Circumstellar absorption lines in the spectrum of alpha Sco B and mass-loss of alpha Sco A. In: Astronomy & Astrophysics. Bd. 70, 1978, S. 227–239, bibcode:1978A&A....70..227K.
- ↑ María Eugenia Veramendi, Jorge Federico González: Spectroscopic study of early-type multiple stellar systems. I. Orbits of spectroscopic binary subsystems. In: Astronomy & Astrophysics. Bd. 563, 2014, Artikel-ID A138, bibcode:2014A&A...563A.138V, doi:10.1051/0004-6361/201322840.
- ↑ Gianni Catanzaro: First spectroscopic analysis of β Scorpii C and β Scorpii E. Discovery of a new HgMn star in the multiple system β Scorpii. In: Astronomy & Astrophysics. Bd. 509, 2010, Artikel-ID A21, bibcode:2010A&A...509A..21C, doi:10.1051/0004-6361/200913332.
- ↑ Thomas C. Van Flandern, Peter Espenschied: Lunar occultations of Beta Scorpii in 1975 and 1976. In: The Astronomical Journal. Bd. 200, 1975, S. 61–67, bibcode:1975ApJ...200...61V, doi:10.1086/153760.
- ↑ Anatoly Miroshnichenko et al.: The 2011 Periastron Passage of the Be Binary δ Scorpii. In: The Astrophysical Journal. Bd. 766 (2), 2013, Artikel-ID 119, bibcode:2013ApJ...766..119M, doi:10.1088/0004-637X/766/2/119, arxiv:1302.4021.
- ↑ William Tango et al.: Orbital elements, masses and distance of λ Scorpii A and B determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy. In: Monthly Notices of the Royal Astronomical Society. Bd. 370 (2), 2006, S. 884–890, bibcode:2006MNRAS.370..884T, doi:10.1111/j.1365-2966.2006.10526.x, arxiv:astro-ph/0605311.
- ↑ Rebekka Grellmann et al.: New constraints on the multiplicity of massive young stars in Upper Scorpius. In: Astronomy & Astrophysics. Bd. 578, 2015, Art.-ID A84, bibcode:2015A&A...578A..84G, doi:10.1051/0004-6361/201219577.
- ↑ a b Andrei Tokovinin: Nearby Quintuple Systems κ Tucanae and ξ Scorpii. In: The Astronomical Journal. Bd. 159 (6), 2020, Artikel-ID 265, bibcode:2020AJ....159..265T, doi:10.3847/1538-3881/ab8af1, arxiv:2005.04057.
- ↑ Andrew Tkachenko et al.: Modelling of σ Scorpii, a high-mass binary with a β Cep variable primary component. In: Monthly Notices of the Royal Astronomical Society. Bd. 442 (1), 2014, S. 616–628, bibcode:2014MNRAS.442..616T, doi:10.1093/mnras/stu885, arxiv:1405.0924.
- ↑ Einzelhelligkeiten aus scheinbarer Gesamthelligkeit V = 4,22 mag (Bright Star Catalogue) und Helligkeitsdifferenz ΔmV = 3,8 (Don Hutter et al.: Surveying the Bright Stars by Optical Interferometry. I. A Search for Multiplicity among Stars of Spectral Types F-K. In: The Astrophysical Journal Supplement Series. Bd. 227 (1), 2016, Artikel-ID 4, bibcode:2016ApJS..227....4H, doi:10.3847/0067-0049/227/1/4, arxiv:1609.05254) berechnet.
- ↑ Sidney B. Parsons et al.: The Fine Guidance Sensor Orbit of the G4 Bright Giant HD 173764. In: The Astronomical Journal. Bd. 129 (3), 2005, S. 1700–1705, bibcode:2005AJ....129.1700P, doi:10.1086/427853.
- ↑ Brian D. Mason et al.: Binary Star Orbits. III. Revisiting the Remarkable Case of Tweedledum and Tweedledee. In: The Astronomical Journal. Bd. 140 (1), 2010, S. 242–252, bibcode:2010AJ....140..242M, doi:10.1088/0004-6256/140/1/242, arxiv:1006.2674.
- ↑ James W. Christy, R. L. Walker, Jr.: MK Classification of 142 Visual Binaries. In: Publications of the Astronomical Society of the Pacific. Bd. 81 (482), 1969, S. 643–649, bibcode:1969PASP...81..643C, doi:10.1086/128831.
- ↑ Nancy Remage Evans et al.: Massive Star Multiplicity: The Cepheid W Sgr. In: The Astronomical Journal. Bd. 137 (3), 2009, S. 3700–3705, bibcode:2009AJ....137.3700E, doi:10.1088/0004-6256/137/3/3700, arxiv:0902.3281.
- ↑ Debra J. Wallace et al.: Hubble Space Telescope Detection of Binary Companions Around Three WC9 Stars: WR 98a, WR 104, and WR 112. In: Interacting Winds from Massive Stars. ASP Conference Proceedings. Edited by Anthony F. J. Moffat and Nicole St-Louis. San Francisco: Astronomical Society of the Pacific. Bd. 260, 2002, S. 407–416, bibcode:2002ASPC..260..407W.
- ↑ Anthony Soulain et al.: SPHERE view of Wolf-Rayet 104. Direct detection of the Pinwheel and the link with the nearby star. In: Astronomy & Astrophysics. Bd. 618, 2018, Artikel-ID A108, bibcode:2018A&A...618A.108S, doi:10.1051/0004-6361/201832817, arxiv:1806.08525.
- ↑ Guillermo Torres et al.: The Hyades Binaries θ1 Tauri and θ2 Tauri: The Distance to the Cluster and the Mass-Luminosity Relation. In: The Astrophysical Journal. Bd. 485 (1), 1997, S. 167–181, bibcode:1997ApJ...485..167T, doi:10.1086/304422.
- ↑ K. B. V. Torres et al.: Spectra disentangling applied to the Hyades binary θ2 Tauri AB: new orbit, orbital parallax and component properties. In: Astronomy & Astrophysics. Bd. 525, 2011, Artikel-ID A50, bibcode:2011A&A...525A..50T, doi:10.1051/0004-6361/201015166, arxiv:1010.5643.
- ↑ J. A. Nemravová et al.: ξ Tauri: a unique laboratory to study the dynamic interaction in a compact hierarchical quadruple system. In: Astronomy & Astrophysics. Bd. 594, 2016, Artikel-ID A55, bibcode:2016A&A...594A..55N, doi:10.1051/0004-6361/201628860.
- ↑ Guillermo Torres: The Multiple System HD 27638. In: The Astronomical Journal. Bd. 131 (3), 2006, S. 1702–1711, bibcode:2006AJ....131.1702T, doi:10.1086/500355, arxiv:astro-ph/0512254.
- ↑ N. Zwahlen et al.: A purely geometric distance to the binary star Atlas, a member of the Pleiades. In: Astronomy & Astrophysics. Bd. 425, 2004, S. L45–L48, bibcode:2004A&A...425L..45Z, doi:10.1051/0004-6361:200400062, arxiv:astro-ph/0408430.
- ↑ Jana Alexandra Nemravová et al.: Properties and nature of Be stars. 27. Orbital and recent long-term variations of the Pleiades Be star Pleione = BU Tauri. In: Astronomy & Astrophysics. Bd. 516, 2010, Artikel-ID A80, bibcode:2010A&A...516A..80N, doi:10.1051/0004-6361/200913885, arxiv:1003.5625.
- ↑ Guillermo Torres et al.: The Hyades Binary Finsen 342 (70 Tauri): A Double-lined Spectroscopic Orbit, the Distance to the Cluster, and the Mass-Luminosity Relation. In: The Astrophysical Journal. Bd. 479 (1), 1997, S. 268–278, bibcode:1997ApJ...479..268T, doi:10.1086/303879.
- ↑ Benjamin F. Lane et al.: The Orbits of the Quadruple Star System 88 Tauri A from PHASES Differential Astrometry and Radial Velocity. In: The Astrophysical Journal. Bd. 669 (2), 2007, S. 1209–1219, bibcode:2007ApJ...669.1209L, doi:10.1086/520877, arxiv:0710.2127.
- ↑ Andrei A. Tokovinin, N. A. Gorynya: New spectroscopic components in multiple systems. IV. In: Astronomy & Astrophysics. Bd. 374 (1), 2001, S. 227–237, bibcode:2001A&A...374..227T, doi:10.1051/0004-6361:20010714.
- ↑ Marco Scardia et al.: Speckle observations with PISCO in Merate – III. Astrometric measurements of visual binaries in 2005 and scale calibration with a grating mask. In: Monthly Notices of the Royal Astronomical Society. Bd. 374 (3), 2007, S. 965–978, bibcode:2007MNRAS.374..965S, doi:10.1111/j.1365-2966.2006.11206.x.
- ↑ D. B. Guenther et al.: Evolutionary Model and Oscillation Frequencies for α Ursae Majoris: A Comparison with Observations. In: The Astrophysical Journal. Bd. 530 (1), 2000, S. L45–L48, bibcode:2000ApJ...530L..45G, doi:10.1086/312473.
- ↑ R. M. Petrie: The spectroscopic binary HD 95638. In: Publications of the Dominion Astrophysical Observatory Victoria. Bd. 11, 1960, S. 259, bibcode:1960PDAO...11..259P.
- ↑ Eric E. Mamajek et al.: Discovery of a Faint Companion to Alcor Using MMT/AO 5 μm Imaging. In: The Astronomical Journal. Bd. 139 (3), 2010, S. 919–925, bibcode:2010AJ....139..919M, doi:10.1088/0004-6256/139/3/919, arxiv:0911.5028.
- ↑ R. Ya. Zhuchkov et al.: Physical parameters and dynamical properties of the multiple system ι UMa (ADS 7114). In: Astronomy Reports. Bd. 56 (7), 2012, S. 512–523, bibcode:2012ARep...56..512Z, doi:10.1134/S1063772912070074.
- ↑ Byeong-Cheol Lee et al.: Long-period Variations in the Radial Velocity of Spectroscopic Binary M Giant μ Ursae Majoris. In: The Astronomical Journal. Bd. 151 (4), 2016, Artikel-ID 106, bibcode:2016AJ....151..106L, doi:10.3847/0004-6256/151/4/106, arxiv:1602.07011.
- ↑ Ning Liu et al.: Tomographic Separation of Composite Spectra. V. The Triple Star System 55 Ursae Majoris In: The Astrophysical Journal. Bd. 485 (1), 1997, S. 350–358, bibcode:1997ApJ...485..350L, doi:10.1086/304418.
- ↑ Yanning Fu, Shulin Ren: Orbit Determination of Double-lined Spectroscopic Binaries by Fitting the Revised Hipparcos Intermediate Astrometric Data. In: The Astronomical Journal. Bd. 139 (5), 2010, S. 1975–1982, bibcode:2010AJ....139.1975R, doi:10.1088/0004-6256/139/5/1975.
- ↑ Albert P. Linnell: A Light Synthesis Study of W Ursae Majoris. In: The Astrophysical Journal. Bd. 374, 1991, S. 307–318, bibcode:1991ApJ...374..307L, doi:10.1086/170120.
- ↑ Nancy Remage Evans et al.: The Orbit of the Close Companion of Polaris: Hubble Space Telescope Imaging, 2007 to 2014. In: The Astrophysical Journal. Bd. 863 (2), 2018, Artikel-ID 187, bibcode:2018ApJ...863..187E, doi:10.3847/1538-4357/aad410, arxiv:1807.06115.
- ↑ Julian R. North et al.: γ2 Velorum: orbital solution and fundamental parameter determination with SUSI. In: Monthly Notices of the Royal Astronomical Society. Bd. 377 (1), 2007, S. 415–424, bibcode:2007MNRAS.377..415N, doi:10.1111/j.1365-2966.2007.11608.x, arxiv:astro-ph/0702375.
- ↑ Antoine Mérand et al.: The nearby eclipsing stellar system δ Velorum. III. Self-consistent fundamental parameters and distance. In: Astronomy & Astrophysics. Bd. 532, 2011, Artikel-ID A50, bibcode:2011A&A...532A..50M, doi:10.1051/0004-6361/201116896, arxiv:1106.2383.
- ↑ David S. Evans: A rediscussion of p Velorum. In: Monthly Notices of the Royal Astronomical Society. Bd. 142, 1969, S. 523–541, bibcode:1969MNRAS.142..523E, doi:10.1093/mnras/142.4.523.
- ↑ E. Victor Garcia et al.: Individual, Model-independent Masses of the Closest Known Brown Dwarf Binary to the Sun. In: The Astrophysical Journal. Bd. 846 (2), 2017, Artikel-ID 97, bibcode:2017ApJ...846...97G, doi:10.3847/1538-4357/aa844f, arxiv:1708.02714.
- ↑ Andrew Tkachenko et al.: Stellar modelling of Spica, a high-mass spectroscopic binary with a β Cep variable primary component. In: Monthly Notices of the Royal Astronomical Society. Bd. 458 (2), 2016, S. 1964–1976, bibcode:2016MNRAS.458.1964T, doi:10.1093/mnras/stw255, arxiv:1601.08069.
- ↑ Marco Scardia et al.: The orbit of the visual binary ADS 8630 (γ Vir). In: Astronomische Nachrichten. Bd. 328 (2), 2007, S. 146 ff., bibcode:2007AN....328..146S, doi:10.1002/asna.200610710.
- ↑ Christian A. Hummel et al.: First Observations with a Co-phased Six-Station Optical Long-Baseline Array: Application to the Triple Star η Virginis. In: The Astronomical Journal. Bd. 125 (5), 2003, S. 2630–2644, bibcode:2003AJ....125.2630H, doi:10.1086/374572.
- ↑ Bradford B. Behr et al.: Stellar Astrophysics with a Dispersed Fourier Transform Spectrograph. II. Orbits of Double-lined Spectroscopic Binaries. In: The Astronomical Journal. Bd. 142 (1), 2011, Artikel-ID 6, bibcode:2011AJ....142....6B, doi:10.1088/0004-6256/142/1/6, arxiv:1104.1447.
- ↑ Guillermo Torres et al.: The Nearby Low-Mass Visual Binary Wolf 424. In: The Astronomical Journal. Bd. 117 (1), 1999, S. 562–573, bibcode:1999AJ....117..562T, doi:10.1086/300708.