Astronomy:NGC 4076
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Short description: Galaxy in the constellation Coma Berenices
NGC 4076 | |
---|---|
SDSS image of 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] |
Helio 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
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 "NASA/IPAC Extragalactic Database". Results for NGC 4076. http://nedwww.ipac.caltech.edu/.
- ↑ "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4076&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.
- ↑ "Revised NGC Data for NGC 4076". http://spider.seds.org/ngc/revngcic.cgi?NGC4076.
- ↑ "New General Catalog Objects: NGC 4050 - 4099". https://cseligman.com/text/atlas/ngc40a.htm#4076.
- ↑ Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal 222: 784–799. doi:10.1086/156198. ISSN 0004-637X. Bibcode: 1978ApJ...222..784G. http://digitalcommons.unl.edu/cgi/viewcontent.cgi?article=1092&context=physicsfacpub.
- ↑ Tifft, W. G.; Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal 231: 23–27. doi:10.1086/157158. ISSN 0004-637X. Bibcode: 1979ApJ...231...23T.
- ↑ 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. doi:10.1086/114494. ISSN 0004-6256. Bibcode: 1987AJ.....94..587B.
- ↑ 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. doi:10.1086/117496. ISSN 0004-6256. Bibcode: 1995AJ....110...46D.
- ↑ 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. doi:10.1086/301103. ISSN 0004-6256. Bibcode: 1999AJ....118.2014W.
- ↑ 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. doi:10.1046/j.1365-8711.2001.04490.x. ISSN 0035-8711. Bibcode: 2001MNRAS.325..693H.
- ↑ Freeland, E.; Stilp, A.; Wilcots, E. (2009-07-01). "H I Observations of Five Groups of Galaxies". The Astronomical Journal 138 (1): 295–304. doi:10.1088/0004-6256/138/1/295. ISSN 0004-6256. Bibcode: 2009AJ....138..295F.
- ↑ 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. doi:10.1111/j.1365-2966.2010.17379.x. ISSN 0035-8711. Bibcode: 2010MNRAS.409.1518F.
- ↑ "NGC 4076". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+4076&QueryType=ned.
- ↑ 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. doi:10.1051/0004-6361/201117461. ISSN 0004-6361. Bibcode: 2011A&A...534A..31G.
- ↑ 15.0 15.1 15.2 "List of supernovae sorted by host name". http://rochesterastronomy.org/snimages/snhnameall.html.
- ↑ "Bright Supernova pages - Most prolific galaxies". http://www.rochesterastronomy.org/snimages/sndupe.html.
- ↑ "Bright Supernovae - 2007.". http://www.rochesterastronomy.org/sn2007/index.html#2007M.
- ↑ 18.0 18.1 "SN 2007M". http://w.astro.berkeley.edu/bait/2007/sn2007M.html.
- ↑ "SN 2007M | Transient Name Server". https://wis-tns.weizmann.ac.il/object/2007M.
- ↑ "2007M - The Open Supernova Catalog" (in en-US). https://sne.space/event/.
- ↑ "Bright Supernovae - 2011.". http://rochesterastronomy.org/sn2011/index.html#2011bc.
- ↑ "SN 2011bc | Transient Name Server". https://wis-tns.weizmann.ac.il/object/2011bc.
- ↑ "2011bc - The Open Supernova Catalog" (in en-US). https://sne.space/event/.
External links
- NGC 4076 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Original source: https://en.wikipedia.org/wiki/NGC 4076.
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