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Hen 2-47 - Versionsgeschichte
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<p><b>Neue Seite</b></p><div>{{Infobox Planetarischer Nebel<br />
| Name = Hen 2-47<br />
| Bild = [[Datei:Hen2-47.jpg|300px]]<br />
| Bildtext = Aufgenommen mit dem [[Hubble-Weltraumteleskop]]<br />
| Sternbild = <br />
| Rek = 10/23/09.143<br />
| Dek = -/60/32/42.21<br />
| Size = <br />
| Caption = Hen 2-47<br />
| z = <br />
| V-Radial = <br />
| magV = <br />
| magB = <br />
| Winkelausdehnung = <br />
| Z-Name = <br />
| Z-mag = <br />
| Z-Spektralklasse = <br />
| LJ = 6600 <br />
| PC = <br />
| Absolut = <br />
| Masse = <br />
| Durchmesser = <br />
| Alter = <br />
| Entdecker = <br />
| Entdeckungsdatum = <br />
| PK = 285-02.1<br />
| IAU = G285.6-02.7<br />
| ESO = 127-16<br />
| GC = <br />
| H = <br />
| h = <br />
| Katalog = <br />
<!-- Quellen --><br />
| RekDekRef = <ref name=simbad>{{SIMBAD|Hen 2-47}}</ref><br />
| zVradRef = <br />
| magRef = <br />
| WinkelRef = <br />
| Z-NameRef = <br />
| Z-magRef = <br />
| Z-SpekRef = <br />
| LJPCRef = <br />
| AbsolutRef = <br />
| MasseRef = <br />
| DurchmesserRef = <br />
| AlterRef = <br />
}}<br />
'''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<br />
| title=Hubble Captures Stars Going Out in Style<br />
| language=en<br />
| url=https://hubblesite.org/contents/news-releases/2007/news-2007-33.html<br />
| publisher=[[Space Telescope Science Institute]]<br />
| date=2007-09-11<br />
| accessdate=2008-12-27}}</ref><br />
Der Nebel wurde von [[Karl Gordon Henize]] 1967 katalogisiert<ref> <br />
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.<br />
<!---<br />
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/><br />
---><br />
== Quellen ==<br />
<references /></div>
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