NGC 4002
| 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
References
- ^ 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. arXiv:1107.3702. 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.
External links
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.