| NGC 4313 | |
|---|---|
SDSS image of NGC 4313. | |
| Observation data ( J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 22m 38.5s [1] |
| Declination | 11° 48′ 03″ [1] |
| Redshift | 0.004813 [1] |
| Heliocentric radial velocity | 1443 km/s [1] |
| Distance | 47.1 Mly (14.45 Mpc) [1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.5 [1] |
| Characteristics | |
| Type | SA(rs)ab [1] |
| Size | ~77,000 ly (23.7 kpc) (estimated) [1] |
| Apparent size (V) | 4.99 x 0.79 [1] |
| Other designations | |
| UGC 07445, VCC 0570, PGC 040105, MCG +02-32-016 [1] | |
NGC 4313 is an edge-on spiral galaxy located about 50 million light-years away [2] in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784. [3] NGC 4313 is a member of the Virgo Cluster [4] [5] and is classified as LINER [2] [6] and as a Seyfert galaxy. [6]
NGC 4313 has undergone ram-pressure stripping in the past. [7]
Black Hole
NGC 4313 may harbor an intermediate-mass black hole with an estimated mass of 200,000 (2*10^5) solar masses. [8]
See also
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4313. Retrieved 2019-08-24.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-08-24.
- ^ "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2019-08-19.
- ^ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area". The Astronomical Journal. 90: 1681–1759. Bibcode: 1985AJ.....90.1681B. doi: 10.1086/113874. ISSN 0004-6256.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-08-24.
- ^ a b Decarli, R.; Gavazzi, G.; Arosio, I.; Cortese, L.; Boselli, A.; Bonfanti, C.; Colpi, M. (2007-10-01). "The census of nuclear activity of late-type galaxies in the Virgo cluster". Monthly Notices of the Royal Astronomical Society. 381 (1): 136–150. arXiv: 0707.0999. Bibcode: 2007MNRAS.381..136D. doi: 10.1111/j.1365-2966.2007.12208.x. ISSN 0035-8711.
- ^ Palous, J.; Taylor, R.; Jachym, P.; Koppen, J. (2018-06-15). "Ram Pressure Stripping Made Easy: An Analytical Approach". Monthly Notices of the Royal Astronomical Society. 479 (4): 4367–4390. arXiv: 1806.05887. Bibcode: 2018MNRAS.479.4367K. doi: 10.1093/mnras/sty1610. S2CID 119245255.
- ^ Davis, Benjamin L.; Soria, Roberto; Graham, Alister W. (2019). "Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies". Monthly Notices of the Royal Astronomical Society. 484 (1): 814. arXiv: 1811.03232. Bibcode: 2019MNRAS.484..814G. doi: 10.1093/mnras/sty3068. S2CID 119303249.
External links
Wikimedia Commons has media related to
NGC 4313.
- NGC 4313 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| NGC 4313 | |
|---|---|
|
SDSS image of NGC 4313. | |
| Observation data ( J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 22m 38.5s [1] |
| Declination | 11° 48′ 03″ [1] |
| Redshift | 0.004813 [1] |
| Heliocentric radial velocity | 1443 km/s [1] |
| Distance | 47.1 Mly (14.45 Mpc) [1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.5 [1] |
| Characteristics | |
| Type | SA(rs)ab [1] |
| Size | ~77,000 ly (23.7 kpc) (estimated) [1] |
| Apparent size (V) | 4.99 x 0.79 [1] |
| Other designations | |
| UGC 07445, VCC 0570, PGC 040105, MCG +02-32-016 [1] | |
NGC 4313 is an edge-on spiral galaxy located about 50 million light-years away [2] in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784. [3] NGC 4313 is a member of the Virgo Cluster [4] [5] and is classified as LINER [2] [6] and as a Seyfert galaxy. [6]
NGC 4313 has undergone ram-pressure stripping in the past. [7]
Black Hole
NGC 4313 may harbor an intermediate-mass black hole with an estimated mass of 200,000 (2*10^5) solar masses. [8]
See also
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4313. Retrieved 2019-08-24.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-08-24.
- ^ "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2019-08-19.
- ^ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area". The Astronomical Journal. 90: 1681–1759. Bibcode: 1985AJ.....90.1681B. doi: 10.1086/113874. ISSN 0004-6256.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-08-24.
- ^ a b Decarli, R.; Gavazzi, G.; Arosio, I.; Cortese, L.; Boselli, A.; Bonfanti, C.; Colpi, M. (2007-10-01). "The census of nuclear activity of late-type galaxies in the Virgo cluster". Monthly Notices of the Royal Astronomical Society. 381 (1): 136–150. arXiv: 0707.0999. Bibcode: 2007MNRAS.381..136D. doi: 10.1111/j.1365-2966.2007.12208.x. ISSN 0035-8711.
- ^ Palous, J.; Taylor, R.; Jachym, P.; Koppen, J. (2018-06-15). "Ram Pressure Stripping Made Easy: An Analytical Approach". Monthly Notices of the Royal Astronomical Society. 479 (4): 4367–4390. arXiv: 1806.05887. Bibcode: 2018MNRAS.479.4367K. doi: 10.1093/mnras/sty1610. S2CID 119245255.
- ^ Davis, Benjamin L.; Soria, Roberto; Graham, Alister W. (2019). "Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies". Monthly Notices of the Royal Astronomical Society. 484 (1): 814. arXiv: 1811.03232. Bibcode: 2019MNRAS.484..814G. doi: 10.1093/mnras/sty3068. S2CID 119303249.
External links
Wikimedia Commons has media related to
NGC 4313.
- NGC 4313 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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