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NGC 4065

NGC 4065
SDSS拍摄的NGC 4065
观测资料(J2000 历元
星座后发座
赤经12h 04m 06.2s[1]
赤纬20° 14′ 06″[1]
红移0.021101[1]
径向速度6326 km/s[1]
距离300 Mly(91 Mpc[1]
属于NGC 4065星系群
视星等 (V)13.58[1]
特征
类型E[1]
大小~120,000 ly(37 kpc[1]
角直径 (V)1.1 x 1.0[1]
其他名称
NGC 4057, MCG +04-29-007, PGC 038156, UGC 07050, VV 179a[1]
参见:星系星系列表

NGC 4065是一个位于后发座椭圆星系,距离地球3亿光年[2][3]。NGC 4065于1785年4月27日由威廉·赫歇尔首次发现,1832年4月29日由约翰·赫歇尔再次发现,并被列为NGC 4057[4]。NGC 4065属于NGC 4065星系团英语NGC 4065 Group[5][6][7],与NGC 4061组成一对交互作用星系[8][5]

参考

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  1. ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 NASA/IPAC Extragalactic Database. Results for NGC 4065. [2019-02-01]. (原始内容存档于2008-12-16). 
  2. ^ Your NED Search Results. ned.ipac.caltech.edu. [2019-02-02]. (原始内容存档于2022-06-29). 
  3. ^ Revised NGC Data for NGC 4065. spider.seds.org. [2019-02-02]. (原始内容存档于2019-02-03). 
  4. ^ New General Catalog Objects: NGC 4050 - 4099. cseligman.com. [2019-01-15]. (原始内容存档于2022-06-30). 
  5. ^ 5.0 5.1 Venkatesan, T. C. A.; Batuski, David J.; Hanisch, Robert J.; Burns, Jack O. Why do head-tail sources exist in poor clusters of galaxies?. The Astrophysical Journal. November 20, 1994, 436: 67–78. Bibcode:1994ApJ...436...67V. ISSN 0004-637X. doi:10.1086/174881 (英语). 
  6. ^ Doe, Stephen M.; Ledlow, Michael J.; Burns, Jack O.; White, Richard A. ROSAT Observations of Five Poor Galaxy Clusters with Extended Radio Sources. The Astronomical Journal. 1995-07-01, 110: 46. Bibcode:1995AJ....110...46D. ISSN 0004-6256. doi:10.1086/117496. 
  7. ^ Freeland, E.; Stilp, A.; Wilcots, E. H I Observations of Five Groups of Galaxies. The Astronomical Journal. 2009-07-01, 138 (1): 295–304. Bibcode:2009AJ....138..295F. ISSN 0004-6256. S2CID 15714969. arXiv:0905.3907可免费查阅. doi:10.1088/0004-6256/138/1/295. 
  8. ^ Batuski, David J.; Hanisch, Robert J.; Burns, Jack O. VLA observations of radio sources in interacting galaxy pairs in poor clusters. The Astronomical Journal. 1992-04-01, 103: 1077–1083. Bibcode:1992AJ....103.1077B. ISSN 0004-6256. doi:10.1086/116126. 

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NGC 4065
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