Quelltext der Seite Hen 2-47

{{Infobox Planetarischer Nebel
|             Name = Hen 2-47
|             Bild = [[File:Hen2-47.jpg|300px]]
|         Bildtext = Aufgenommen mit dem [[Hubble-Weltraumteleskop]]
|        Sternbild = 
|              Rek = 10/23/09.143
|              Dek = -/60/32/42.21
|             Size = 
|          Caption = Hen 2-47
|                z = 
|         V-Radial = 
|             magV = 
|             magB = 
| Winkelausdehnung = 
|           Z-Name = 
|            Z-mag = 
| Z-Spektralklasse = 
|               LJ = 6600 
|               PC = 
|          Absolut = 
|            Masse = 
|      Durchmesser = 
|            Alter = 
|        Entdecker = 
| Entdeckungsdatum = 
|               PK = 285-02.1
|              IAU = G285.6-02.7
|              ESO = 127-16
|               GC = 
|                H = 
|                h = 
|          Katalog = 
<!-- Quellen -->
|        RekDekRef = <ref name=simbad>{{cite web
  | title=SIMBAD Astronomical Database
  | work=Results for Hen 2-47
  | url=http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Hen+2-47
  | accessdate=2008-12-27}}</ref>
|         zVradRef = 
|           magRef = 
|        WinkelRef = 
|        Z-NameRef = 
|         Z-magRef = 
|        Z-SpekRef = 
|          LJPCRef = 
|       AbsolutRef = 
|         MasseRef = 
|   DurchmesserRef = 
|         AlterRef = 
}}
'''Hen 2-47''' (auch ''Hen 2-47'') ist ein junger [[planetarischer Nebel]] im Sternbild [[Kiel des Schiffs|Carina]], der 6600 [[Lichtjahr]]e entfernt ist.<ref name=hubblesite>{{cite web
  | title=Hubble Captures Stars Going Out in Style
  | url=http://hubblesite.org/newscenter/archive/releases/nebula/planetary/2007/33/image/a/
  | accessdate=2008-12-27}}</ref>
Der Nebel wurde von [[Karl Gordon Henize]] 1967 katalogisiert.<ref>	
Karl G.	Henize: ''Observations of Southern Planetary Nebulae'', {{bibcode|1967ApJS...14..125H}}</ref>, worin eine von Margaret Mayall 1951 publizierte Beobachtung<ref>M. W. Mayall: ''New Peculiar Spectra'', {{bibcode|1951BHarO.920...32M}}</ref> referenziert ist. 
<!---
Hen 2-47 contains six lobes of [[gas]] and dust that suggest that the central [[star]] of the nebula ejected material at least three times in three different directions. During each ejection, the star fired off a narrow pair jets of gas pointed in opposite directions, eventually giving the nebula the shape it has at present.<ref name=hubblesite/>
--->
== Quellen ==
<references />