NGC 2328位于船尾座,是一个透鏡狀星系。其星团较大,较为年轻[3]。NGC 2328距离地球约5900万光年[3]

NGC 2328
哈勃空间望远镜拍摄的NGC 2328
观测资料(J2000 曆元
星座船尾座
赤经07h 02m 36.193s[1]
赤纬-42° 04′ 06.88″[1]
紅移0.003930[2]
徑向速度1176.0 km/s[2]
距离59 Mly(18 Mpc[3]
视星等 (V)12.55[4]
视星等 (B)13.16[4]
絕對星等 (V)−18.5[3]
特征
类型(R')SAB0?[5]
其他名称
MCG-07-15-002、​PGC 20046[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 [2022-06-03]. ISSN 0004-6256. doi:10.1086/498708. (原始内容存档于2022-04-02). 
  2. ^ 2.0 2.1 2.2 NGC 2328. SIMBAD. 斯特拉斯堡天文資料中心. [2021-02-02]. 
  3. ^ 3.0 3.1 3.2 3.3 Väisänen, Petri; Barway, Sudhanshu; Randriamanakoto, Zara. Star Clusters in a Nuclear Star Forming Ring: The Disappearing String of Pearls. The Astrophysical Journal. 2014, 797 (2): L16. Bibcode:2014ApJ...797L..16V. S2CID 118491641. arXiv:1411.3385 . doi:10.1088/2041-8205/797/2/L16. 
  4. ^ 4.0 4.1 Search specification: NGC 2328. HyperLeda. Université Claude Bernard Lyon 1. [2021-02-02]. (原始内容存档于2020-09-16). 
  5. ^ Results for object NGC 2328 (NGC 2328). NASA/IPAC Extragalactic Database. California Institute of Technology. [2021-02-02]. (原始内容存档于2022-06-03).