Three-point correlations of galaxy clusters

Details Three-point correlations of galaxy clusters Three-point correlations of galaxy clusters

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344...75t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 344, Sept. 1, 1989, p. 75-88. Research supported by NASA, NSF, Johns Hopkin

Statistics

Computation

51

Computational Astrophysics, Galactic Clusters, Astronomical Catalogs, Correlation, Spatial Distribution

Scientific paper

A relation between two- and three-point correlation functions similar to that of galaxies is presently established by estimating the irreducible angular three-point correlation function of Abell clusters in distance classes 5 and 6, for Galactic latitudes below 40 deg. The shape of the three-point correlation function is fully consistent with the quadratic scaling law found by Groth and Peebles (1977) for galaxies. The three-point correlation function is inconsistent with the expectations from biasing.

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