NGC 4076
Appearance
(Redirected from SN 2011bc)
NGC 4076 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 12h 04m 32.5s[1] |
Declination | 20° 12′ 18″[1] |
Redshift | 0.020728[1] |
Heliocentric radial velocity | 6214 km/s[1] |
Distance | 291 Mly (89.1 Mpc)[1] |
Group or cluster | NGC 4065 Group |
Apparent magnitude (V) | 14.35[1] |
Characteristics | |
Type | Sa[1] |
Size | ~103,000 ly (31.6 kpc) (estimated)[1] |
Apparent size (V) | 0.9 x 0.9[1] |
Other designations | |
UGC 07061, PGC 038209, MCG +03-31-034[1] |
NGC 4076 is a spiral galaxy located 290 million light-years away[2] in the constellation Coma Berenices.[3] The galaxy was discovered by astronomer William Herschel on April 27, 1785[4] and is a member of the NGC 4065 Group.[5][6][7][8][9][10][11][12]
NGC 4076 is classified as a LINER galaxy.[13][14]
NGC 4076 has been host to two type Ia supernovae.[15][16] The first, SN 2007M was first observed on December 24, 2006.[15][17][18] However, it was discovered on January 14, 2007.[18][19][20] The second, SN 2011bc was discovered on April 1, 2011.[15][21][22][23]
References
[edit]- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4076. Retrieved 2019-02-09.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-02-10.
- ^ "Revised NGC Data for NGC 4076". spider.seds.org. Retrieved 2019-02-10.
- ^ "New General Catalog Objects: NGC 4050 - 4099". cseligman.com. Retrieved 2019-02-03.
- ^ Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ...222..784G. doi:10.1086/156198. ISSN 0004-637X.
- ^ Tifft, W. G.; Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T. doi:10.1086/157158. ISSN 0004-637X.
- ^ Burns, Jack O.; Hanisch, Robert J.; White, Richard A.; Nelson, Eric R.; Morrisette, Kim A.; Moody, J. Ward (1987-09-01). "A VLA 20 CM survey of poor groups of galaxies". The Astronomical Journal. 94: 587–617. Bibcode:1987AJ.....94..587B. doi:10.1086/114494. ISSN 0004-6256.
- ^ Doe, Stephen M.; Ledlow, Michael J.; Burns, Jack O.; White, Richard A. (1995-07-01). "ROSAT Observations of Five Poor Galaxy Clusters with Extended Radio Sources". The Astronomical Journal. 110: 46. Bibcode:1995AJ....110...46D. doi:10.1086/117496. ISSN 0004-6256.
- ^ White, Richard A.; Bliton, Mark; Bhavsar, Suketu P.; Bornmann, Patricia; Burns, Jack O.; Ledlow, Michael J.; Loken, Christen (1999-11-01). "A Catalog of Nearby Poor Clusters of Galaxies". The Astronomical Journal. 118 (5): 2014–2037. arXiv:astro-ph/9907283. Bibcode:1999AJ....118.2014W. doi:10.1086/301103. ISSN 0004-6256. S2CID 73667751.
- ^ Helsdon, Stephen F.; Ponman, Trevor J.; O'Sullivan, Ewan; Forbes, Duncan A. (2001-08-01). "X-ray luminosities of galaxies in groups". Monthly Notices of the Royal Astronomical Society. 325 (2): 693–706. arXiv:astro-ph/0103293. Bibcode:2001MNRAS.325..693H. doi:10.1046/j.1365-8711.2001.04490.x. ISSN 0035-8711. S2CID 17732882.
- ^ Freeland, E.; Stilp, A.; Wilcots, E. (2009-07-01). "H I Observations of Five Groups of Galaxies". The Astronomical Journal. 138 (1): 295–304. arXiv:0905.3907. Bibcode:2009AJ....138..295F. doi:10.1088/0004-6256/138/1/295. ISSN 0004-6256. S2CID 15714969.
- ^ Freeland, E.; Sengupta, C.; Croston, J. H. (2010-12-01). "Quantifying the importance of ram-pressure stripping in a galaxy group at 100 Mpc". Monthly Notices of the Royal Astronomical Society. 409 (4): 1518–1524. arXiv:1007.3286. Bibcode:2010MNRAS.409.1518F. doi:10.1111/j.1365-2966.2010.17379.x. ISSN 0035-8711. S2CID 119216322.
- ^ "NGC 4076". sim-id. Retrieved 2019-02-10.
- ^ Gavazzi, G.; Savorgnan, G.; Fumagalli, Mattia (2011-10-01). "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. Bibcode:2011A&A...534A..31G. doi:10.1051/0004-6361/201117461. ISSN 0004-6361. S2CID 73621726.
- ^ a b c "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-02-02.
- ^ "Bright Supernova pages - Most prolific galaxies". www.rochesterastronomy.org. Retrieved 2019-02-10.
- ^ "Bright Supernovae - 2007". www.rochesterastronomy.org. Retrieved 2019-02-10.
- ^ a b "SN 2007M". w.astro.berkeley.edu. Retrieved 2019-02-10.
- ^ "SN 2007M | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-02-10.
- ^ "2007M - The Open Supernova Catalog". Archived from the original on 2016-09-17. Retrieved 2019-02-10.
- ^ "Bright Supernovae - 2011". rochesterastronomy.org. Retrieved 2019-02-10.
- ^ "SN 2011bc | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-02-10.
- ^ "2011bc - The Open Supernova Catalog". Archived from the original on 2016-09-17. Retrieved 2019-02-10.
External links
[edit]Wikimedia Commons has media related to NGC 4076.
- NGC 4076 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images