| 词条 | NGC 1850 |
| 释义 |
| image = |caption=A Hubble Space Telescope (HST) image of NGC 1850. |credit=HST/NASA/ESA. | name = NGC 1850 | epoch = J2000.0 | ra = {{RA|5|8|45}}[1] | dec = {{DEC|-68|45|42}}[1] | dist_ly = | dist_pc = | appmag_v = 9.0 | size_v = 3.4′ | radius_ly = | absmag_v = | constellation name = Dorado | notes = | names = NGC 1850, ESO 056-SC070, h 2780, GC 1060 }}NGC 1850 is a double cluster and a super star cluster in the Dorado constellation, located in the Large Magellanic Cloud at the distance of 168,000 ly (51,510 pc). It was discovered by James Dunlop in 1826. It is an unusual cluster of stars because the distribution of its stars is like a globular cluster, but unlike the globular clusters of the Milky Way it is composed of young stars. The only similar object in the Milky Way is Westerlund 1.[2] References{{commons category}}1. ^1 {{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 1850 | url=http://nedwww.ipac.caltech.edu/ | accessdate=2007-04-03}} {{star-cluster-stub}}2. ^{{cite journal | author = Gallagher | author2 = Grebel | last-author-amp = yes | date = 2002 | title = Extragalactic Star Clusters: Speculations on the Future | journal = Extragalactic Star Clusters, IAU Symposium | volume = 207 | page = 207 | bibcode = 2002IAUS..207..745G|arxiv = astro-ph/0109052 }} 4 : Dorado (constellation)|Open clusters|NGC objects|Large Magellanic Cloud |
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