Cosmic strings and the formation of clusters of galaxies

Details Cosmic strings and the formation of clusters of galaxies Cosmic strings and the formation of clusters of galaxies

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138..105j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 105-112.

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4

Cosmology, Dark Matter, Galactic Clusters, Galactic Evolution, String Theory, Adiabatic Conditions, Computational Astrophysics, Universe

Scientific paper

The relation between the mean separation d of clusters of galaxies and their mean richness N is found to be well represented by d = 3.4N2/3. Both this observed result and the Bahcall-Soneira relation (that is, the spatial correlations of clusters of galaxies are increased with their richness) are well explained by the cosmic string picture, lending support to the cosmic-string theory.

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