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NGC 770

From Wikipedia, the free encyclopedia
Galaxy in the constellation Aries
NGC 770
NGC 770 and NGC 772 imaged by theSloan Digital Sky Survey
Observation data (J2000epoch)
ConstellationAries
Right ascension01h 59m 13.64260s[1]
Declination+18° 57′ 16.7211″[1]
Heliocentric radial velocity2,543[2]
Distance120 Mly (36.7 Mpc)[2]
Characteristics
TypeE3:[3]
Apparent size (V)0.587 × 0.399″[4]
Other designations
UGC 1463, PGC 7517[5]

NGC 770 is anelliptical galaxy in theconstellation Aries. It is around 120[2] million light years from the Milky Way and has a diameter of around 36,000 ly.[3] NGC 770 is gravitationally linked toNGC 772.[6] The galaxy was discovered on November 3, 1855 byR. J. Mitchell.[7][8][9]

References

[edit]
  1. ^abBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abcCappellari, Michele; et al. (May 2011)."The ATLAS3D project - I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria".Monthly Notices of the Royal Astronomical Society.413 (2):813–836.arXiv:1012.1551.Bibcode:2011MNRAS.413..813C.doi:10.1111/j.1365-2966.2010.18174.x.S2CID 15391206.
  3. ^abde Vaucouleurs, G.; et al. (1991).Third Reference Catalogue of Bright Galaxies. 3.9. New York:Springer-Verlag.Bibcode:1991rc3..book.....D.
  4. ^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.S2CID 18913331.
  5. ^"NGC 770".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-01-13.
  6. ^Tully, R. Brent (May 2015). "Galaxy Groups: A 2MASS Catalog".The Astronomical Journal.149 (5): 14.arXiv:1503.03134.Bibcode:2015AJ....149..171T.doi:10.1088/0004-6256/149/5/171.S2CID 119285986. 171.
  7. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2019-12-12.
  8. ^"Revised NGC Data for NGC 770".spider.seds.org. Retrieved2019-12-12.
  9. ^Ford, Dominic."The galaxy NGC 770 - In-The-Sky.org".in-the-sky.org. Retrieved2019-12-12.

External links

[edit]
  • Media related toNGC 770 at Wikimedia Commons
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