The structure of the Universe traced by rich clusters of galaxies.

Details The structure of the Universe traced by rich clusters of galaxies. The structure of the Universe traced by rich clusters of galaxies.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sucg.conf...63e&link_type=abstract

Workshop on Studying the Universe with Clusters of Galaxies, p. 63 - 76

Computer Science

Clusters Of Galaxies: Universe, Large-Scale Structure: Universe, Clusters Of Galaxies: Space Distribution

Scientific paper

The authors study the whole-sky distribution of Abell clusters of galaxies up to distance z ≍ 0.1. The distribution of clusters, superclusters and voids show the presence of the characteristic scale of 130 h-1Mpc in the supercluster-void network, found earlier by Broadhurst et al. (1990) from 1-dimensional study. This scale is detected in the distribution of Abell clusters of richness both R = 0 and R ≥ 1. The authors compare the distribution of ACO clusters with that of APM clusters. The APM clusters determine a smaller scale - 100 h-1Mpc. The authors discuss the possible reasons of this difference.

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