NGC 7836

NGC 7836
NGC 7836
	SDSS image of NGC 7836.
Observation data (J2000 epoch)
Constellation	Andromeda
Right ascension	00h 08m 01.6s
Declination	33° 04′ 15″
Redshift	0.016358
Helio radial velocity	4904 km/s
Distance	260 Mly (80 Mpc)
Apparent magnitude (V)	14.4
Characteristics
Type	Irr?, Sb
Size	~83,000 ly (25.5 kpc) (estimated)
Apparent size (V)	0.9 x 0.5
Other designations
	CGCG 498-79, CGCG 499-51, IRAS 00054+3247, KUG 0005+327, Mrk 336, NPM1G +32.0005, PGC 608, UGC 65

NGC 7836 is an irregular^[2]^[3] or spiral galaxy located about 260 million light-years away^[2] in the constellation of Andromeda. It was discovered by astronomer Lewis Swift on September 20, 1885.^[3]

References

^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j "NASA/IPAC Extragalactic Database". Results for NGC 7836. Retrieved 2019-03-11.
^ ^a ^b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-03-11.
^ ^a ^b ^c "New General Catalog Objects: NGC 7800 – 7840". cseligman.com. Retrieved 2017-08-11.
^ Garcia, A. M. (1993-07-01). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
^ Vettolani, G.; Baiesi Pillastrini, G. C. (1987-03-01). "Alignments of galaxies in the Perseus supercluster". Astronomy and Astrophysics. 175: 9–14. Bibcode:1987A&A...175....9V. ISSN 0004-6361.
^ Cabanela, J. E.; Aldering, G. (1998-09-01). "Galaxy Alignments in the Pisces-Perseus Supercluster Revisited". The Astronomical Journal. 116 (3): 1094–1117. Bibcode:1998AJ....116.1094C. doi:10.1086/300484. ISSN 0004-6256.