NGC 1792

NGC 1792 is a spiral galaxy located in the Columba constellation. It was discovered by James Dunlop on October 4, 1826. It is located about 36.4 million light-years away.[3]

Hubble image of NGC 1792
NGC 1792
Observation data (J2000 epoch)
ConstellationColumba
Right ascension05h 05m 14.454s[1]
Declination−37° 58′ 50.70″[1]
Redshift0.004059[2]
Helio radial velocity1214.3 km/s[2]
Distance36.4 Mly (11.17 Mpc)[3]
Apparent magnitude (V)10.18[2]
Apparent magnitude (B)10.68[2]
Characteristics
TypeSA(rs)bc
Other designations
PGC 16709, ESO 305-6, MCG -6-12-004, ESO LV3050060, IRAS 05035-3802[2]

References
  1. 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: 1163–1183. doi:10.1086/498708. ISSN 0004-6256.
  2. "NGC 1792". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-12.
  3. Tully, R. Brent; Courtois, Hélène M.; Sorce, Jenny G. (2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. 50.

http://www.skyfactory.org/deepskycatalogue/db_list.asp?q=(Name~contains~NGC1792)


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