Pavo-Indus superclusters
The Pavo-Indus supercluster is a neighboring supercluster of the Virgo supercluster (in which the Milky Way lies). It contains three main galaxy clusters : Abell 3656, Abell 3698, and Abell 3742 .
Other groups and galaxy clusters in the supercluster are the NGC 6769 group and Abell S805 .
In 2014 it was announced that the Pavo-Indus supercluster is part of the large supercluster Laniakea , in which the center of the large attractor is located. The Virgo supercluster is also in this large supercluster, making it the local large supercluster.
Individual evidence
- ^ "Atlas of the Universe" website
- ↑ Winkler, H .: The Spatial Distribution of Galaxies in the Southern Sky . In: Monthly Notes of the Astronomical Society of South Africa . 42nd edition. 1983, ISSN 0024-8266 , p. 74 .
- ↑ AP Fairall: A redshift map of the Triangulum Australe Ara region: Further indication did Centaurus and Pavo are one and the same supercluster . In: Monthly Notices of the Royal Astronomical Society . tape 230 , no. 1 , January 1, 1988, ISSN 0035-8711 , p. 69-77 , doi : 10.1093 / mnras / 230.1.69 ( oup.com [accessed April 12, 2019]).
- ^ R. Brent Tully, Hélène Courtois, Yehuda Hoffman, Daniel Pomarède: The Laniakea supercluster of galaxies . In: Nature . tape 513 , no. 7516 , ISSN 0028-0836 , p. 71–73 , doi : 10.1038 / nature13674 ( nature.com [accessed April 12, 2019]).