NGC 3486是一个位于小狮座中间棒旋星系,距离地球2740万光年[3],为SAB(r)c类星系[5]。它属于西佛星系,有一个活动星系核,但未检测到其发射的无线电波,可能星系内部黑洞质量较小,不到100万太阳质量[6]

NGC 3486
NGC 3486
哈勃空间望远镜拍摄的NGC 3486
观测资料(J2000 历元
星座小狮座
赤经11h 00m 23.946s[1]
赤纬+28° 58′ 29.35″[1]
红移+0.004113 ± 0.000003[2]
径向速度+681[3] km/s
距离27.4 Mly (8.41 Mpc)[3]
视星等 (V)10.5[4]
特征
类型SAB(r)c[5]
角直径 (V)7.1' × 5.3'
其他名称
UGC 6079
参见:星系星系列表

参考

  1. ^ 1.0 1.1 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. The Two Micron All Sky Survey (2MASS). The Astronomical Journal. 1 February 2006, 131: 1163–1183 [2022-06-22]. ISSN 0004-6256. doi:10.1086/498708. (原始内容存档于2022-04-02). 
  2. ^ Wegner, Gary; et al, Redshifts for 2410 Galaxies in the Century Survey Region, The Astronomical Journal, December 2001, 122 (6): 2893–2900, Bibcode:2001AJ....122.2893W, arXiv:astro-ph/0109101 , doi:10.1086/323915. 
  3. ^ 3.0 3.1 3.2 Crook, Aidan C.; et al, Groups of Galaxies in the Two Micron All Sky Redshift Survey, The Astrophysical Journal, February 2007, 655 (2): 790–813, Bibcode:2007ApJ...655..790C, arXiv:astro-ph/0610732 , doi:10.1086/510201. 
  4. ^ NASA/IPAC Extragalactic Database. Results for NGC 3486. [2006-11-21]. (原始内容存档于2011-05-14). 
  5. ^ 5.0 5.1 Conselice, C. J., The Symmetry, Color, and Morphology of Galaxies, Publications of the Astronomical Society of the Pacific, November 1997, 109: 1251–1255, Bibcode:1997PASP..109.1251C, arXiv:astro-ph/9710234 , doi:10.1086/134004. 
  6. ^ Maoz, Dan, Low-luminosity active galactic nuclei: are they UV faint and radio loud?, Monthly Notices of the Royal Astronomical Society, June 2007, 377 (4): 1696–1710, Bibcode:2007MNRAS.377.1696M, arXiv:astro-ph/0702292 , doi:10.1111/j.1365-2966.2007.11735.x. 

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