Astronomy:NGC 2032
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Short description: Emission nebula in the constellation Dorado
Emission nebula | |
---|---|
Observation data: epoch | |
Right ascension | 05h 35m 20.0s[1] |
Declination | −67° 34′ 36″[1] |
Constellation | Dorado |
Designations | ESO 56-EN160, Seagull Nebula |
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
- ↑ 1.0 1.1 "Object: NGC 2032". Spider.Seds. http://spider.seds.org/ngc/revngcic.cgi?NGC2032.
- ↑ "NGC 2032". astroanarchy.zenfolio. 27 October 2010. http://astroanarchy.zenfolio.com/p62690868/h3BCA41CC#h3bca41cc.
- ↑ "NGC 2032 (= EN in LMC)". cseligman. http://cseligman.com/text/atlas/ngc20.htm#2032.
- ↑ "Your NED Search Results". http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+2032&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
Original source: https://en.wikipedia.org/wiki/NGC 2032.
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