NGC 4002
Appearance
NGC 4002 | |
---|---|
![]() SDSS image of NGC 4002. | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 57m 59.3s[1] |
Declination | 23° 12′ 07″[1] |
Redshift | 0.021959[1] |
Heliocentric radial velocity | 6583 km/s[1] |
Distance | 310 Mly (94 Mpc)[1] |
Apparent magnitude (V) | 14.96[1] |
Absolute magnitude (B) | -22.76[1] |
Characteristics | |
Type | S0-a[1] |
Size | ~155,300 ly (47.62 kpc) (estimated)[1] |
Apparent size (V) | 0.8′ × 0.4′[1] |
Other designations | |
CGCG 127-116, MCG +04-28-104, PGC 037635[1] |
NGC 4002 is a lenticular galaxy located 310 million light-years away[2] in the constellation Leo. It was discovered on April 10, 1785, by astronomer William Herschel.[3] NGC 4002 forms a pair with the galaxy NGC 4003 known as [T2015] nest 102886,[4] and is part of the Coma Supercluster.[5][6]
NGC 4002 is a quasar candidate according to Simbad,[7] and is host to a supermassive black hole with an estimated mass of 9 × 108 M☉.[8]
See also
[edit]References
[edit]- ^ a b c d e f g h i j k "Results for object NGC 4002". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 2025-07-08.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2025-07-08.
- ^ "New General Catalog Objects: NGC 4000 - 4049". cseligman.com. Retrieved 2025-07-08.
- ^ Tully, R. Brent (2015-04-28). "GALAXY GROUPS: A 2MASS CATALOG". The Astronomical Journal. 149 (5): 171. arXiv:1503.03134. doi:10.1088/0004-6256/149/5/171. ISSN 1538-3881.
- ^ 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. doi:10.1086/114001. ISSN 0004-6256.
- ^ Gavazzi, G.; Savorgnan, G.; Fumagalli, Mattia (October 2011). "The complete census of optically selected AGNs in the Coma supercluster: the dependence of AGN activity on the local environment". Astronomy and Astrophysics. 534: A31. doi:10.1051/0004-6361/201117461. ISSN 0004-6361.
- ^ "NGC 4002". simbad.u-strasbg.fr. Retrieved 2025-07-08.
- ^ 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.