The distribution of clusters of galaxies within 300 Mpc/h and the crossover to an isotropic and homogeneous universe

Astronomy and Astrophysics – Astronomy

Scientific paper

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Galactic Clusters, Galactic Structure, Spatial Distribution, Universe, Cosmology, Inhomogeneity, Local Group (Astronomy)

Scientific paper

Firm evidence is presented from clusters of galaxies in the Abell and ACO galaxies for the spatial convergence of a cosmological dipole which increases with distance up to about 180/h Mpc, then bends and remains flat within the sample depth, while the monopole continues to grow linearly with distance up to a maximum sample depth of 300/h Mpc. It is at that point more than 5 times above the dipole level; this monopole growth behavior demonstrates that the dipole's convergence is real, rather than due to the depth incompleteness of the sample. An analysis of the behavior of the dipole as a function of distance suggests that a nonnegligible fraction of the peculiar acceleration responsible for the Local Group motion comes from greater depths than concluded from earlier studies.

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