M101星系群

M101星系群
風車星系是M101星系群中最亮的星系。
觀測數據(曆元J2000
星座大熊座
赤经14h 04m[1][2]
赤纬+54° 31′[1][2]
最亮的成員風車星系[3][1][2]
星系的數量6-9[4][3][1][2]
其它名稱
NGC 5457 Group, LGG 371,[1]
NOGG H 758,[2] NOGG P1 766,[2]
NOGG P2 781[2]
參見:星系群星系团星系團列表

M101星系群是在大熊座內的一個結構鬆散的星系群,這個星系群是以其中最亮的星系M101命名的,群中其他的星系大多是風車星系的伴星系[4][3][1][2]。這個星系群本身也是室女座超星系團(也就是本超星系團)眾多成員之一[5]

成員

下表是在鄰近的星系目錄中一向被確認的小組成員[4],是由Fouque等人量測的[3],獅子座星系團(LGG)目錄[1],和這三個星系群表是Giuricin等人建立的鄰近光學星系樣品[2]

M101星系群的成員
名稱 類型[6] R.A. (J2000)[6] Dec. (J2000)[6] 紅移 (km/s)[6] 視星等[6]
風車星系(M101) SAB(rs)cd 14h 03m 12.6s +54° 20′ 57″ 241 ± 2 8.3
NGC 5204 SA(s)m 13h 29m 36.5s +58° 25′ 07″ 201 ± 1 11.7
NGC 5474 SA(s)cd pec 14h 05m 01.6s +53° 39′ 44″ 273 ± 9 11.3
NGC 5477 SA(s)m 14h 05m 33.2s +54° 27′ 39″ 304 ± 5 14.4
NGC 5585 SAB(s)d 14h 19m 48.2s +56° 43′ 45″ 305 ± 3 11.2
UGC 8837 IB(s)m 13h 54m 45.8s +53° 54′ 03″ 144 ± 3 13.8
UGC 9405 Im 14h 35m 24.4s +57° 15′ 19″ 222 ± 6 17

其它可能的成員(只從上述參考的目錄中列出一兩個名單)包括不規則星系 NGC 5238UGC 8508

鄰近的集團

M51星系群,包含車輪星系(M51)向日葵星系(M63)[4][3][1][2],位在M101星系群的西南方,NGC 5866星系群在西北方[7]。這三個星系團的距離(對集團中的星系進行獨立的測量)是相似的,建議M51星系團、M101星系團、和NGC 5866星系確實團都是更大星系團鬆散和延伸結構的一部份[7]但是,多數認定星系團的方法(包括前述所參考和援引的資料)都認為這三個星系團是完全分開的集團。

相關條目

參考資料

  1. ^ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 A. Garcia. General study of group membership. II - Determination of nearby groups. Astronomy and Astrophysics Supplement. 1993, 100: 47–90 [2021-02-07]. (原始内容存档于2019-12-13). 
  2. ^ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 G. Giuricin, C. Marinoni, L. Ceriani, A. Pisani. Nearby Optical Galaxies: Selection of the Sample and Identification of Groups. Astrophysical Journal. 2000, 543: 178–194 [2009-04-07]. doi:10.1086/317070. (原始内容存档于2019-01-21). 
  3. ^ 3.0 3.1 3.2 3.3 3.4 P. Fouque, E. Gourgoulhon, P. Chamaraux, G. Paturel. Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members. Astronomy and Astrophysics Supplement. 1992, 93: 211–233 [2021-02-07]. (原始内容存档于2019-12-13). 
  4. ^ 4.0 4.1 4.2 4.3 R. B. Tully. Nearby Galaxies Catalog. Cambridge: Cambridge University Press. 1988. ISBN 0-521-35299-1. 
  5. ^ R. B. Tully. The Local Supercluster. Astrophysical Journal. 1982, 257: 389–422 [2009-04-07]. doi:10.1086/159999. (原始内容存档于2018-09-30). 
  6. ^ 6.0 6.1 6.2 6.3 6.4 NASA/IPAC Extragalactic Database. Results for various galaxies. [2006-10-15]. (原始内容存档于2018-12-25). 
  7. ^ 7.0 7.1 L. Ferrarese, H. C. Ford, J. Huchra, R. C. Kennicutt Jr., J. R. Mould, S. Sakai, W. L. Freedman, P. B. Stetson, B. F. Madore, B. K. Gibson, J. A. Graham, S. M. Hughes, G. D. Illingworth, D. D. Kelson, L. Macri, K. Sebo, N. A. Silbermann. A Database of Cepheid Distance Moduli and Tip of the Red Giant Branch, Globular Cluster Luminosity Function, Planetary Nebula Luminosity Function, and Surface Brightness Fluctuation Data Useful for Distance Determinations. Astrophysical Journal Supplement. 2000, 128: 431–459 [2009-04-07]. doi:10.1086/313391. (原始内容存档于2007-10-15). 

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