NGC 80
Appearance
NGC 80 | |
---|---|
![]() SDSS image of NGC 80 | |
Observation data (J2000 epoch) | |
Constellation | Andromeda |
Right ascension | 00h 21m 10.865s[1] |
Declination | +22° 21′ 26.11″[1] |
Redshift | 0.019006 |
Heliocentric radial velocity | 5698[2] |
Distance | 260.76 ± 66.60 Mly (79.950 ± 20.421 Mpc)[2] |
Group or cluster | NGC 80 group[3] |
Apparent magnitude (V) | 12.07[2] |
Apparent magnitude (B) | 13.7[4] |
Absolute magnitude (V) | -22.38[2] |
Characteristics | |
Type | SA0−[2] |
Size | 166,900 ly (51,160 pc)[2] |
Apparent size (V) | 2.2′ × 2.002′[2] |
Other designations | |
UGC 203, MCG+04-02-004, PGC 1351[4] |
NGC 80 is a lenticular galaxy located in the constellation Andromeda. It is interacting with NGC 47 and NGC 68, and is the brightest cluster galaxy of the NGC 80 group, a galaxy group named after it.[3]
References
- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256.
- ^ a b c d e f g "NED Results for NGC 0080". NASA/IPAC Extragalactic Database. Retrieved 18 February 2017.
- ^ a b Silchenko, Olga K.; Afanasiev, Victor L. (2008). "Stellar populations and galaxy evolution in the NGC 80 group". arXiv:0807.0334 [astro-ph].
- ^ a b "NGC 80". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 18 February 2017.
External links