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Hercules Supercluster

Hercules Supercluster ( SCl 160 , English Hercules Superclusters ) - a supercluster of galaxies in the constellation Hercules . It consists of two neighboring, interconnected, superclusters of galaxies, which are often referred to as the northern and southern parts of a single supercluster of Hercules. The northern part is located at a distance of 400 million light years, a little further, at a distance of 500 million light years, lies the southern part of the supercluster [2] .

Hercules Supercluster
Supercluster of Galaxies
Her.gif
Observational data
( Age J2000.0 )
Constellation (s)Hercules
The brightest clusterHercules Cluster
Supercluster Main Axis100 Mpc (326 million light years )
Distance400-500 million light years
Redshift0.0304-0.0414 [1]
Research history
DesignationsSCl 160

In the 1930s, Harlow Shapley studied the distribution structure of galaxies in the constellation Hercules, and was probably the first to know about the existence of a supercluster in this area. However, this was not confirmed until the 1970s. In 1976, Massimo Tarenhi suggested that the A2151 cluster is part of a single supercluster, and at a conference on the large-scale structure of the Universe in Estonia in 1977, he, together with V. Typhus, G. Chinsarini, S. Rood and L. Thompson, presented evidence that the supercluster appears in this region [2] .

Compared to other local superclusters, the Hercules supercluster is considered especially large, reaching approximately 330 million light-years in diameter. The redshifts of the galaxies entering the supercluster are between 0.0304 and 0.0414 [1] .

The supercluster includes Abell 2147 , the Hercules Cluster (Abell 2151) and Abell 2152 [3] [4] . It was found that the distant clusters Abell 2197 and Abell A2199, connected by extremely long filaments of galaxies, also belong to the supercluster of Hercules [4] . Abell 2162 in the constellation Northern Crown is also a member of the supercluster [5] .

The Hercules supercluster is located near the supercluster of Veronica's Hair , both of which are parts of the Great Wall of CfA2 [6] .

Notes

  1. ↑ 1 2 Kopylova, FG; Kopylov, AI Investigation of properties of galaxy clusters in the Hercules supercluster region (Eng.) // Astronomy Letters: journal. - 2013 .-- Vol. 39 , no. 1 . - P. 1-16 . - DOI : 10.1134 / S1063773712120043 . - .
  2. ↑ 1 2 The Hercules Superclusters (neopr.) . Atlasoftheuniverse.com. Date of treatment November 19, 2011.
  3. ↑ Program 48: Hercules Supercluster (neopr.) . Tdc-www.harvard.edu. Date of treatment November 19, 2011.
  4. ↑ 1 2 Voids and Superclusters (unopened) (link not available) . Netfiles.uiuc.edu. Date of treatment November 19, 2011. Archived June 30, 2012.
  5. ↑ Einasto, M .; Einasto, J .; Tago, E .; Müller, V .; Andernach, H. Optical and X-Ray Clusters as Tracers of the Supercluster-Void Network. I. Superclusters of Abell and X-Ray Clusters (Eng.) // The Astronomical Journal : journal. - IOP Publishing , 2001. - Vol. 122 , no. 5 . - P. 2222-2242 . - DOI : 10.1086 / 323707 . - . - arXiv : astro-ph / 0012536 .
  6. ↑ Clusters and Superclusters of Galaxies (neopr.) . Ned.ipac.caltech.edu. Date of treatment November 19, 2011.

Links

  • SIMBAD - Hercules Supercluster
  • transcendens.info - Hercules Supercluster
Source - https://ru.wikipedia.org/w/index.php?title= Hercules Supercluster&oldid = 100079271


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