The Spatial Distribution of Nearby Galaxy Clusters in the Northern and Southern Galactic Hemispheres

Astronomy and Astrophysics – Astrophysics

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20 pages

Scientific paper

We compare the spatial distributions of galaxy clusters in the northern and southern galactic hemispheres, and the Abell and ACO clusters distributions. We perform a statistical (correlation and cluster) analysis of a sample of Abell and ACO galaxy clusters in the southern galactic hemisphere. We compare these results with a symmetric sample at northern galactic latitude taken from Postman et al. (1992). For the northern sample, we substantially confirm the results of Postman et al. We find that the two-point spatial correlation function of northern and southern clusters is comparable, with mean correlation length 19.6 Mpc and slope -1.8 positive up to about 45 Mpc. Percolation properties are remarkably similar in the northern and southern cluster samples. We give also a catalog of superclusters. In the south galactic hemisphere the main feature is a very rich, extended supercluster in the Horologium region at a redshift 0.06, near to a large void.

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