玉夫座长城

玉夫座長城（紅移是Z=0.03）是一個相對靠近銀河系的星系超級結構（星系長城），也是一般所謂的玉夫座超星系團[1][2]。這個超級結構也稱為"南方長城"、"大南方城牆"、"南牆"，以與北方長城或直接稱為長城的CfA2長城相呼應。它的結構在'紅移空間'的維度長8000 km/s，寬5000 km/s，深1000 km/s[3][4]。

包括玉夫座長城的近域宇宙（local universe）。
包括玉夫座超星系團的近域宇宙。
2MASS的距離圖，包括近域宇宙主要的玉夫座超星系團。

參考資料
  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 , Bibcode：2010ApJ...714.1715F , arXiv:1001.3692 ,
  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: Bibcode：1990MNRAS.247P..21F （页面存档备份，存于） (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） ; Fairall, A. P., Paverd, W. R., & Ashley, R. P. ; Bibcode：1994ASPC...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 Bibcode：1995Ap&SS.230..225F
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