NGC 1850
| NGC 1850 | |
|---|---|
 | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 5h 8m 45s[1] |
| Declination | −68° 45′ 42″[1] |
| Apparent magnitude (V) | 9.0 |
| Apparent dimensions (V) | 3.4′ |
| Physical characteristics | |
| Other designations | NGC 1850, ESO 056-SC070, h 2780, GC 1060 |
| Associations | |
| Constellation | Dorado |
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
- ^ a b "NASA/IPAC Extragalactic Database". Results for NGC 1850. Retrieved 2007-04-03.
- ^ Gallagher; Grebel (2002). "Extragalactic Star Clusters: Speculations on the Future". Extragalactic Star Clusters, IAU Symposium. 207: 207. arXiv:astro-ph/0109052. Bibcode:2002IAUS..207..745G.
{{cite journal}}: Unknown parameter|last-author-amp=ignored (|name-list-style=suggested) (help)
External links
Media related to NGC 1850 at Wikimedia Commons
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |