NGC 4459

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]

NGC 4459
The central dust lane of NGC 4459 as imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 29m 00.0s[1]
Declination13° 58′ 42″[1]
Redshift0.003976/1192 km/s[1]
Distance52,500,000 ly
Group or clusterVirgo Cluster
Apparent magnitude (V)11.32 [1]
Characteristics
TypeSA0^+(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]

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]

2MASS image of NGC 4459
gollark: <@!330678593904443393> You are in group 1.
gollark: <@356107472269869058> You are in group "", a new group.
gollark: <@!402456897812168705> You are in group one.
gollark: <@!341618941317349376> You are in Group -A.
gollark: I'm sure you'd like to think so.

See also

References
  1. "NASA/IPAC Extragalactic Database". Results for NGC 4459. Retrieved 2017-08-20.
  2. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-08-22.
  3. Rojas, Sebastián García. "Galaxy NGC 4459 - Galaxy in Coma Berenices Constellation · Deep Sky Objects Browser". DSO Browser. Retrieved 2017-08-22.
  4. "New General Catalog Objects: NGC 4450 - 4499". cseligman.com. Retrieved 2017-08-18.
  5. "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2017-08-22.
  6. 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. arXiv:0712.4189. doi:10.1086/529019.
  7. 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. arXiv:0811.1381. Bibcode:2009AJ....137.3053Y. doi:10.1088/0004-6256/137/2/3053.
  8. "List of black hole candidates". www.johnstonsarchive.net. Retrieved 2017-08-20.
  9. "2.8662 Astronomical unit - Wolfram|Alpha Results". m.wolframalpha.com. Retrieved 2017-10-21.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.