玉夫座长城红移是Z=0.03)是一个相对靠近银河系星系超级结构(星系长城),也是一般所谓的玉夫座超星系团[1][2]。这个超级结构也称为"南方长城"、"大南方城墙"、"南墙",以与北方长城或直接称为长城的CfA2长城相呼应。它的结构在'红移空间'的维度长8000 km/s,宽5000 km/s,深1000 km/s[3][4]

包括玉夫座长城的近域宇宙(local universe)。
包括玉夫座超星系团的近域宇宙。
2MASS的距离图,包括近域宇宙主要的玉夫座超星系团。

参考资料

编辑
  1. ^ Taotao Fang1, David A. Buote1, Philip J. Humphrey1, Claude R. Canizares2, Luca Zappacosta3, Roberto Maiolino4, Gianpiero Tagliaferri5 and Fabio Gastaldello; CONFIRMATION OF X-RAY ABSORPTION BY WARM-HOT INTERGALACTIC MEDIUM IN THE SCULPTOR WALL; 2010 ApJ 714 1715 , doi:10.1088/0004-637X/714/2/1715 , Bibcode2010ApJ...714.1715F , , [1]
  2. ^ Fairall, A. P., Palumbo, G. G. C., Vettolani, G., Kauffman, G., Jones, A., & Baiesi-Pillastrini, G., Largescale Structure in the Universe - Plots from the Updated Catalogue of Radial Velocities of Galaxies and the Southern Redshift Catalogue Journal: R.A.S. MONTHLY NOTICES V.247, NO.2/NOV15, P. 23P, 1990. Bibliographic Code: Bibcode1990MNRAS.247P..21F [2]页面存档备份,存于互联网档案馆) (slices 8 and 10 under SGH)
  3. ^ Unveiling large-scale structures behind the Milky Way. Astronomical Society of the Pacific Conference Series, Vol. 67; Proceedings of a workshop at the Observatoire de Paris-Meudon; 18–21 January 1994; San Francisco: Astronomical Society of the Pacific (ASP); c1994; edited by Chantal Balkowski and R. C. Kraan-Korteweg, p.21 ; Visualization of Nearby Large-Scale Structures页面存档备份,存于互联网档案馆) ; Fairall, A. P., Paverd, W. R., & Ashley, R. P. ; Bibcode1994ASPC...67...21F
  4. ^ 'Astrophysics and Space Science', Volume 230, Issue 1-2, pp. 225-235 Large-Scale Structures in the Distribution of Galaxies 08/1995 Bibcode1995Ap&SS.230..225F