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NGC 3073

Coordinates:Sky map10h 00m 52.042s, +55° 37′ 08.17″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Ursa Major
NGC 3073
NGC 3073 imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationUrsa Major
Right ascension10h 00m 52.042s[1]
Declination+55° 37′ 08.17″[1]
Redshift0.003933[2]
Heliocentric radial velocity1177 km/s[2]
Distance65 Mly (20 Mpc)[3]
Group orclusterNGC 3079 Group
Apparent magnitude (V)13.40[3]
Apparent magnitude (B)14.07[3]
Characteristics
TypeSAB0[3]
Size~40,300 ly (12.36 kpc) (estimated)[4]
Apparent size (V)1.2′ × 1.1′[4]
Other designations
HOLM 156B,UGC 5374,MCG +09-17-007,Mrk 131,PGC 28974,CGCG 265-054[2][4]

NGC 3073 is a dwarflenticular galaxy in the constellationUrsa Major.[5][6][7] It is at a distance of about 65 millionlight-years (20megaparsecs) fromEarth.[3] NGC 3073 was discovered byGerman-British astronomerWilliam Herschel on 1 April 1790.[8]

NGC 3073 belongs to theNGC 3079 Group (also known asLGG 188), which contains six galaxies.[9] The other galaxies in the group are NGC 3079, UGC 5421, UGC 5479, UGC 5459, andUGC 5460.[10] The galaxies NGC 3073 and NGC 3079 are also listed together asHolm 156 inErik Holmberg'sA Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[11]

Wikimedia Commons has media related toNGC 3073.

Gallery

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  • NGC 3073 imaged by SDSS
    NGC 3073 imaged bySDSS

See also

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References

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  1. ^abSkrutskie, 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.
  2. ^abc"NGC 3073".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-09-13.
  3. ^abcdeGil de Paz, Armando; et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies".The Astrophysical Journal Supplement Series.173 (2):185–255.arXiv:astro-ph/0606440.Bibcode:2007ApJS..173..185G.doi:10.1086/516636.S2CID 119085482.
  4. ^abc"Results for object NGC 1285".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved18 November 2024.
  5. ^"SIMBAD".simbad.u-strasbg.fr. France:University of Strasbourg. Retrieved2020-09-10.
  6. ^"A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies"(PDF).CERN (PDF).Astrophysical Journal Letters.
  7. ^Irwin, J. A.; Seaquist, E. R. (1991)."INIS Repository Search - Single Result".International Nuclear Information System.The Astrophysical Journal:111–130. Retrieved2020-09-10.
  8. ^Seligman, Courtney."New General Catalogue Objects: NGC 3073".Celestial Atlas. Retrieved18 November 2024.
  9. ^Shafi, N.; Oosterloo, T. A.;Morganti, R.; Colafrancesco, S.; Booth, R. (2015-12-01)."The "shook up" galaxy NGC 3079: the complex interplay between HI, activity and environment".Monthly Notices of the Royal Astronomical Society.454 (2):1404–1415.arXiv:1509.00350.Bibcode:2015MNRAS.454.1404S.doi:10.1093/mnras/stv2034.S2CID 55595738.
  10. ^Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups".Astronomy and Astrophysics Supplement Series.100: 47.Bibcode:1993A&AS..100...47G.
  11. ^Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems".Annals of the Observatory of Lund.6: 1.Bibcode:1937AnLun...6....1H.

External links

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