SDSS image of NGC 4061. NGC 4065 can be seen to the left of the image.
Observation data (J2000 epoch)
Constellation
Coma Berenices
Right ascension
12h 04m 01.5s[1]
Declination
20° 13′ 56″[1]
Redshift
0.024027[1]
Heliocentric radial velocity
7203 km/s[1]
Distance
310 Mly (94 Mpc)[1]
Group or cluster
NGC 4065 Group
Apparent magnitude (V)
14.12[1]
Characteristics
Type
E[1]
Size
~120,000 ly (37 kpc) (estimated)[1]
Apparent size (V)
1.2 x 0.9[1]
Other designations
NGC 4055, MCG +04-29-006, PGC 038146, UGC 07044, VV 179b[1]
NGC 4061 is an elliptical galaxy located 310 light-years away[2] in the constellation Coma Berenices.[3] It was discovered by astronomer William Herschel on April 27, 1785. It was rediscovered by John Herschel on April 29, 1832. It is listed both as NGC 4061 and NGC 4055.[4] NGC 4061 is a member of the NGC 4065 Group[5][6][7][8][9][10][11][12][13] and forms an interacting[14][15] pair with its companion, NGC 4065[8][14] as evidenced by distortions in their optical isophotes.[15][9]
NGC 4061 is classified as a radio galaxy[7][15][9][16][17][18][11][19] with a Fanaroff and Riley classification of type I.[20]
^ abcdefghij"NASA/IPAC Extragalactic Database". Results for NGC 4061. Retrieved 2019-01-20.
^"Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-01-21.
^"Revised NGC Data for NGC 4061". spider.seds.org. Retrieved 2019-01-21.
^"New General Catalog Objects: NGC 4050 - 4099". cseligman.com. Retrieved 2019-01-15.
^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.
^ abJaffe, W.; Gavazzi, G.; Valentijn, E. (1986-02-01). "Radio continuum survey of the Coma/A1367 supercluster. I - 610 MHz observations of CGCG galaxies in four groups". The Astronomical Journal. 91: 199–203. Bibcode:1986AJ.....91..199J. doi:10.1086/114000. ISSN 0004-6256.
^ abBurns, 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.
^ abcDoe, 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.
^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.
^ abCroston, J. H.; Sengupta, C.; Freeland, E. (2010-12-21). "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.
^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.
^Freeland, E.; Stilp, A.; Wilcots, E. (2009-07-01). "HI 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.
^ abBatuski, David J.; Hanisch, Robert J.; Burns, Jack O. (1992-04-01). "VLA observations of radio sources in interacting galaxy pairs in poor clusters". The Astronomical Journal. 103: 1077–1083. Bibcode:1992AJ....103.1077B. doi:10.1086/116126. ISSN 0004-6256.
^ abcVenkatesan, T. C. A.; Batuski, David J.; Hanisch, Robert J.; Burns, Jack O. (November 20, 1994). "Why do head-tail sources exist in poor clusters of galaxies?". The Astrophysical Journal. 436: 67–78. Bibcode:1994ApJ...436...67V. doi:10.1086/174881. ISSN 0004-637X.
^Zaninetti, L. (2007-04-01). "Physical mechanisms that shape the morphologies of extragalactic jets". Revista Mexicana de Astronomía y Astrofísica. 43: 59–87. arXiv:astro-ph/0610400. Bibcode:2007RMxAA..43...59Z. ISSN 0185-1101.
^Zaninetti, Lorenzo (2009-03-06). "A turbulent model for the surface brightness of extragalactic jets". Revista Mexicana de Astronomía y Astrofísica. 45: 25–53. arXiv:0903.1170. Bibcode:2009RMxAA..45...25Z.
^Gavazzi, Giuseppe; Fumagalli, Mattia; Cucciati, Olga; Boselli, Alessandro (July 2010). "A snapshot on galaxy evolution occurring in the Great Wall: the role of Nurture at z=0". Astronomy and Astrophysics. 517: A73. arXiv:1003.3795. Bibcode:2010A&A...517A..73G. doi:10.1051/0004-6361/201014153. ISSN 0004-6361. S2CID 55001713.
^"NGC 4061". sim-id. Retrieved 2019-01-21.
^Capetti, A.; Massaro, F.; Baldi, R. D. (2017-02-01). "FRICAT: A FIRST catalog of FR I radio galaxies". Astronomy and Astrophysics. 598: A49. arXiv:1610.09376. Bibcode:2017A&A...598A..49C. doi:10.1051/0004-6361/201629287. ISSN 0004-6361. S2CID 119216781.
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