Astronomy:NGC 4065

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Short description: Galaxy in the constellation Coma Berenices
NGC 4065
SDSS NGC 4065.jpg
SDSS image of NGC 4065. The halo of NGC 4061 can be seen at the right of the image.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 04m 06.2s[1]
Declination20° 14′ 06″[1]
Redshift0.021101[1]
Helio radial velocity6326 km/s[1]
Distance300 Mly (91 Mpc)[1]
Group or clusterNGC 4065 Group
Apparent magnitude (V)13.58[1]
Characteristics
TypeE[1]
Size~120,000 ly (37 kpc) (estimated)[1]
Apparent size (V)1.1 x 1.0[1]
Other designations
NGC 4057, MCG +04-29-007, PGC 038156, UGC 07050, VV 179a[1]

NGC 4065 is an elliptical galaxy located 300 million light-years away[2] in the constellation Coma Berenices.[3] The galaxy was discovered by astronomer William Herschel on April 27, 1785. It was then rediscovered by John Herschel on April 29, 1832 and was listed as NGC 4057.[4] NGC 4065 is the brightest[5][6][7][8] member of the NGC 4065 Group.[5][9][10][6][11][12][13][7][14][15]

NGC 4065 is a companion of NGC 4061.[10][16] The two galaxies form an interacting[16][6] pair, as evidenced by distortions in their optical isophotes.[6][11]

It is classified as a radio galaxy.[11][6]

See also

References

  1. ↑ 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 4065. http://nedwww.ipac.caltech.edu/. 
  2. ↑ "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4065&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. 
  3. ↑ "Revised NGC Data for NGC 4065". http://spider.seds.org/ngc/revngcic.cgi?NGC4065. 
  4. ↑ "New General Catalog Objects: NGC 4050 - 4099". https://cseligman.com/text/atlas/ngc40a.htm#4065. 
  5. ↑ 5.0 5.1 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. 
  6. ↑ 6.0 6.1 6.2 6.3 6.4 Venkatesan, 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?" (in en). The Astrophysical Journal 436: 67–78. doi:10.1086/174881. ISSN 0004-637X. Bibcode: 1994ApJ...436...67V. 
  7. ↑ 7.0 7.1 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. 
  8. ↑ Gottlieb, Steve. "Astronomy-Mall: Adventures In Deep Space NGC objects 4001-4999". https://www.astronomy-mall.com/Adventures.In.Deep.Space/NGC%204000%20-%204999%20(11-30-17).htm. 
  9. ↑ 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. 
  10. ↑ 10.0 10.1 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. 
  11. ↑ 11.0 11.1 11.2 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. 
  12. ↑ 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. 
  13. ↑ 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. 
  14. ↑ 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. 
  15. ↑ "NGC 4065". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC++4065&NbIdent=query_hlinks&Coord=12+04+06.167%2B20+14+05.95&parents=5&submit=parents&children=1&siblings=32&hlinksdisplay=h_all. 
  16. ↑ 16.0 16.1 Batuski, 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. doi:10.1086/116126. ISSN 0004-6256. Bibcode: 1992AJ....103.1077B. 

External links



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