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NASA NTRS · 19890064589

Three-point correlations of galaxy clusters

Abstract

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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BibTeXRIS

Toth, Gabor, Hollosi, Joseph, Szalay, Alexander S.. 1989-09-01. Three-point correlations of galaxy clusters. https://ntrs.nasa.gov/citations/19890064589

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