NGC 3619是一个位于大熊座透鏡狀星系[4],1790年3月18日由威廉·赫歇爾发现[5],气体含量较大[4]

NGC 3619
SDSS拍摄的NGC 3619
观测资料(J2000 曆元
星座大熊座
赤经11h 19m 21.621s[1]
赤纬+57° 45′ 27.66″[1]
紅移0.005240[2]
徑向速度1567 ± 47 km/s[2]
距离87 Mly(26.8 Mpc[3]
视星等 (B)12.6[2]
特征
类型(R)SA(s)0+[4]
其他名称
UGC 6330、​MCG+10-16-115、​PGC 34641[2]
參見: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 [2022-06-25]. ISSN 0004-6256. doi:10.1086/498708. (原始内容存档于2022-04-02). 
  2. ^ 2.0 2.1 2.2 2.3 NGC 3619. SIMBAD. 斯特拉斯堡天文資料中心. [2021-06-01]. 
  3. ^ Cappellari, Michele; et al. The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria. Monthly Notices of the Royal Astronomical Society. 11 May 2011, 413 (2): 813–836. Bibcode:2011MNRAS.413..813C. S2CID 15391206. arXiv:1012.1551 . doi:10.1111/j.1365-2966.2010.18174.x. 
  4. ^ 4.0 4.1 4.2 Sil'chenko, Olga K.; Moiseev, Alexei V.; Egorov, Oleg V. The Gas Kinematics, Excitation, and Chemistry, in Connection with Star Formation, in Lenticular Galaxies. The Astrophysical Journal Supplement Series. 2019, 244 (1): 6. Bibcode:2019ApJS..244....6S. S2CID 197431133. arXiv:1907.07261 . doi:10.3847/1538-4365/ab3415. 
  5. ^ Seligman, Courtney. New General Catalogue objects: NGC 3600 - 3649. cseligman.com. [2021-06-01]. (原始内容存档于2019-02-18). 

外部链接