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NGC 1850 - 版本历史
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<p><b>新页面</b></p><div>{{Infobox open cluster<br />
| image = [[File:NGC1850.jpg|280px|]]<br />
|caption=[[哈伯太空望遠鏡]]拍攝NGC 1850影像<br />
|credit=HST/[[NASA]]/[[ESA]].<br />
| name = NGC 1850<br />
| epoch = J2000.0<br />
| ra = {{RA|5|8|45}}<ref name="ned">{{cite web<br />
| title=NASA/IPAC Extragalactic Database<br />
| work=Results for NGC 1850<br />
| url=http://nedwww.ipac.caltech.edu/<br />
| accessdate=2007-04-03<br />
| archive-date=2011-05-14<br />
| archive-url=https://web.archive.org/web/20110514100451/http://nedwww.ipac.caltech.edu/<br />
| dead-url=no<br />
}}</ref><br />
| dec = {{DEC|-68|45|42}}<ref name="ned" /><br />
| dist_ly = <br />
| dist_pc = <br />
| appmag_v = 9.0<br />
| size_v = 3.4&prime;<br />
| radius_ly =<br />
| absmag_v =<br />
| constellation name = [[劍魚座]]<br />
| notes = <br />
| names = [[NGC天體表|NGC]]&nbsp;1850, ESO 056-SC070, h 2780, GC 1060 }}<br />
<br />
'''NGC 1850'''是在距離地球16.8萬光年（51510秒差距）的[[大麥哲倫星系]]中，由兩個星團組成的[[超星團]]，在天球上位於[[劍魚座]]。NGC 1850由[[詹姆士·敦洛普]]發現於1826年8月3日。NGC 1850是一個不尋常的星團，因為該星團內的恆星分布與球狀星團類似，但和銀河系的球狀星團不同的是其成員星是年輕恆星。銀河系中唯一與NGC 1850類似的天體只有[[維斯特盧1]]<ref name=gallagher02>{{cite journal<br />
| author = Gallagher<br />
| author2 = Grebel<br />
| last-author-amp = yes <br />
| date = 2002<br />
| title = Extragalactic Star Clusters: Speculations on the Future<br />
| journal = Extragalactic Star Clusters, IAU Symposium<br />
| volume = 207<br />
| page = 207<br />
| bibcode = 2002IAUS..207..745G<br />
|arxiv = astro-ph/0109052 }}</ref>。<br />
<br />
[[File:NGC 1850.jpg|thumb|left|250 px|[[欧洲南方天文台]]拍攝的NGC 1850影像，可見該星團周圍的雲氣分布。]]<br />
<br />
== 參考資料 ==<br />
{{Reflist}}<br />
<br />
{{NGCReference|1850}}<br />
<br />
{{star-cluster-stub}}<br />
[[Category:劍魚座NGC天體|1850]]<br />
[[Category:大麥哲倫星系]]<br />
[[Category:疏散星团]]<br />
[[Category:1826年發現的天體]]</div>
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