Astronomy:NGC 4673
From HandWiki
| NGC 4673 | |
|---|---|
| File:250px SDSS image of NGC 4673. | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 45m 34.7s[1] |
| Declination | 27° 03′ 39″[1] |
| Redshift | 0.022856[1] |
| Helio radial velocity | 6852 km/s[1] |
| Distance | 317 Mly (97.2 Mpc) |
| Apparent magnitude (V) | 13.87[1] |
| Absolute magnitude (B) | -21.96[1] |
| Characteristics | |
| Type | E1-2[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 an elliptical galaxy located 317 million light-years away[2] in the constellation Coma Berenices. It was discovered on April 6, 1785, by astronomer William Herschel.[3] NGC 4673 part of a group of 11 galaxies, known as [T2015] nest 100111, which is also known as the NGC 4692 Group[4] and is part of the Coma Supercluster.[5][6]
NGC 4673 is host to a supermassive black hole with an estimated mass of 7.2 × 108 M☉,[7] and a population of 750 globular clusters.[8]
See also
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "Results for object NGC 4673". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+4585.
- ↑ "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC%204673&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA%20or%20Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
- ↑ "New General Catalog Objects: NGC 4650 - 4699". https://cseligman.com/text/atlas/ngc46a.htm#4673.
- ↑ Tully, R. Brent (May 2015). "Galaxy Groups: A 2MASS Catalog" (in en). The Astronomical Journal 149 (5): 171. doi:10.1088/0004-6256/149/5/171. ISSN 0004-6256. Bibcode: 2015AJ....149..171T. https://ui.adsabs.harvard.edu/abs/2015AJ....149..171T/abstract.
- ↑ Gregory, S. A.; Thompson, L. A. (June 1978). "The Coma/A1367 supercluster and its environs" (in en). The Astrophysical Journal 222: 784. doi:10.1086/156198. ISSN 0004-637X. Bibcode: 1978ApJ...222..784G. http://adsabs.harvard.edu/doi/10.1086/156198.
- ↑ Jaffe, W.; Gavazzi, G. (February 1986). "Radio continuum survey of the coma/A1367 supercluster. II. 1.5 GHz observations of 396 CGCG galaxies." (in en). The Astronomical Journal 91: 204–216. doi:10.1086/114001. ISSN 0004-6256. Bibcode: 1986AJ.....91..204J. https://ui.adsabs.harvard.edu/abs/1986AJ.....91..204J/abstract.
- ↑ Arzoumanian, Zaven; Baker, Paul T.; Brazier, Adam; Brook, Paul R.; Burke-Spolaor, Sarah; Becsy, Bence; Charisi, Maria; Chatterjee, Shami et al. (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. doi:10.3847/1538-4357/abfcd3. ISSN 0004-637X. Bibcode: 2021ApJ...914..121A.
- ↑ 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?" (in en). The Astrophysical Journal 772 (2): 82. doi:10.1088/0004-637X/772/2/82. ISSN 0004-637X. Bibcode: 2013ApJ...772...82H. https://ui.adsabs.harvard.edu/abs/2013ApJ...772...82H/abstract.
External links
Template:NGC objects:4500-4999
