| Emission nebula | |
|---|---|
| π Image | |
| Observation data: epoch | |
| Right ascension | 05h 35m 20.0s[1] |
| Declination | β67Β° 34β² 36β³[1] |
| Constellation | Dorado |
| Designations | ESO 56-EN160, Seagull Nebula |
| See also: Lists of nebulae | |
NGC 2032 (also known as ESO 56-EN160 and the Seagull Nebula) is an emission nebula in the Dorado constellation and near the supershell LMC-4[2] and it consists of NGC 2029, NGC 2035 and NGC 2040. It was first discovered by James Dunlop on 27 September 1826, and John Herschel rerecorded it on 2 November 1834.[3] NGC 2032 is located in the Large Magellanic Cloud.[4]
References
[edit]- ^ a b "Object: NGC 2032". Spider.Seds. Retrieved 9 October 2017.
- ^ "NGC 2032". astroanarchy.zenfolio. 27 October 2010. Retrieved 9 October 2017.
- ^ "NGC 2032 (= EN in LMC)". cseligman. Retrieved 9 October 2017.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-23.
Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_2032&oldid=1250728034"
