Astronomy:NGC 4459
From HandWiki
Short description: Galaxy in the constellation Coma Berenicies
NGC 4459 | |
---|---|
The central dust lane of NGC 4459 as imaged by the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 12h 29m 00.0s[1] |
Declination | 13° 58′ 42″[1] |
Redshift | 0.003976/1192 km/s[1] |
Distance | 52,500,000 ly |
Group or cluster | Virgo Cluster |
Apparent magnitude (V) | 11.32 [1] |
Characteristics | |
Type | SA0^+(r), LINER[1] |
Size | ~ 54,770 ly |
Apparent size (V) | 3.5 x 2.7[1] |
Other designations | |
CGCG 70-116, IRAS 12264+1415, MCG 2-32-83, PGC 41104, UGC 7614, VCC 1154 [1] |
NGC 4459 is a lenticular galaxy located about 50 million light-years away[2] in the constellation of Coma Berenices.[3] NGC 4459 is also classified as a LINER galaxy.[2] NGC 4459 was discovered by astronomer William Herschel on January 14, 1787.[4] NGC 4459 is a member of the Virgo Cluster.[5]
Physical characteristics
Dust disk
NGC 4459 has a central flocculent dust disk that surrounds an inner ring.[6][7] Also, there appears to be evidence of ongoing star formation in the disk .[7]
Super massive black hole
NGC 4459 has a supermassive black hole with an estimated mass of roughly 70 million suns (7×107 M☉). Its diameter is estimated to be around 2.87 astronomical units[8] (266.4 million mi).[9]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "NASA/IPAC Extragalactic Database". Results for NGC 4459. http://nedwww.ipac.caltech.edu/.
- ↑ 2.0 2.1 "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4459&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
- ↑ Rojas, Sebastián García. "Galaxy NGC 4459 - Galaxy in Coma Berenices Constellation · Deep Sky Objects Browser" (in en). https://dso-browser.com/deep-sky/5505/ngc-4459/galaxy.
- ↑ "New General Catalog Objects: NGC 4450 - 4499" (in en-US). http://cseligman.com/text/atlas/ngc44a.htm#4459.
- ↑ "Detailed Object Classifications". https://ned.ipac.caltech.edu/cgi-bin/NEDatt?objname=NGC+4459.
- ↑ Young, Lisa M.; Bureau, Martin; Cappellari, Michele (23 December 2007). "Structure and Kinematics of Molecular Disks in Fast‐Rotator Early‐Type Galaxies". The Astrophysical Journal 676: 317–334. doi:10.1086/529019.
- ↑ 7.0 7.1 Young, Lisa M.; Bendo, George J.; Lucero, Danielle M. (13 January 2009). "Mid- to Far-Infrared Emission and Star Formation in Early-Type Galaxies". The Astronomical Journal 137 (2): 3053–3070. doi:10.1088/0004-6256/137/2/3053. Bibcode: 2009AJ....137.3053Y.
- ↑ "List of black hole candidates". http://www.johnstonsarchive.net/relativity/bhctable.html.
- ↑ "2.8662 Astronomical unit - Wolfram|Alpha Results". http://m.wolframalpha.com/input/?i=2.8662+Astronomical+unit.
External links
- NGC 4459 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Original source: https://en.wikipedia.org/wiki/NGC 4459.
Read more |