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NGC 4673

From Wikipedia, the free encyclopedia
Galaxy in the constellation Coma Berenices
NGC 4673
SDSS image of NGC 4673.
Observation data (J2000epoch)
ConstellationComa Berenices
Right ascension12h 45m 34.7s[1]
Declination27° 03′ 39″[1]
Redshift0.022856[1]
Heliocentric radial velocity6852 km/s[1]
Distance317 Mly (97.2 Mpc)
Apparent magnitude (V)13.87[1]
Absolute magnitude (B)-21.96[1]
Characteristics
TypeE1-2[1]
Size~75,100 ly (23.04 kpc) (estimated)[1]
Apparent size (V)1.0′ × 0.9′[1]
Other designations
UGC 07933, MRK 0656, CGCG 159-070, MCG +05-30-073, PGC 043008[1]

NGC 4673 is anelliptical galaxy located 317 millionlight-years away[2] in theconstellationComa Berenices. It was discovered on April 6, 1785, by astronomerWilliam Herschel.[3] NGC 4673 is part of a group of 11 galaxies, known as [T2015] nest 100111, which is also known as theNGC 4692 Group[4] and is part of theComa Supercluster.[5][6]

NGC 4673 is host to asupermassive black hole with an estimated mass of 7.2 × 108M,[7] and a population of 750globular clusters.[8]

See also

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References

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  1. ^abcdefghij"Results for object NGC 4673".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved2025-09-19.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2025-09-19.
  3. ^"New General Catalog Objects: NGC 4650 - 4699".cseligman.com. Retrieved2025-09-19.
  4. ^Tully, R. Brent (May 2015)."Galaxy Groups: A 2MASS Catalog".The Astronomical Journal.149 (5): 171.arXiv:1503.03134.Bibcode:2015AJ....149..171T.doi:10.1088/0004-6256/149/5/171.ISSN 0004-6256.
  5. ^Gregory, S. A.; Thompson, L. A. (June 1978)."The Coma/A1367 supercluster and its environs".The Astrophysical Journal.222: 784.Bibcode:1978ApJ...222..784G.doi:10.1086/156198.ISSN 0004-637X.
  6. ^Jaffe, W.; Gavazzi, G. (February 1986)."Radio continuum survey of the coma/A1367 supercluster. II. 1.5 GHz observations of 396 CGCG galaxies".The Astronomical Journal.91:204–216.Bibcode:1986AJ.....91..204J.doi:10.1086/114001.ISSN 0004-6256.
  7. ^Arzoumanian, Zaven; Baker, Paul T.; Brazier, Adam; Brook, Paul R.; Burke-Spolaor, Sarah; Becsy, Bence; Charisi, Maria; Chatterjee, Shami; Cordes, James M.; Cornish, Neil J.; Crawford, Fronefield; Cromartie, H. Thankful; Decesar, Megan E.; Demorest, Paul B.; Dolch, Timothy (2021-06-01)."The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc".The Astrophysical Journal.914 (2): 121.arXiv:2101.02716.Bibcode:2021ApJ...914..121A.doi:10.3847/1538-4357/abfcd3.ISSN 0004-637X.
  8. ^Harris, William E.; Harris, Gretchen L. H.; Alessi, Matthew (August 2013)."A Catalog of Globular Cluster Systems: What Determines the Size of a Galaxy's Globular Cluster Population?".The Astrophysical Journal.772 (2): 82.arXiv:1306.2247.Bibcode:2013ApJ...772...82H.doi:10.1088/0004-637X/772/2/82.ISSN 0004-637X.

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