The fractal properties of the two-dimensional distribution of galaxy clusters.

Details The fractal properties of the two-dimensional distribution of galaxy clusters. The fractal properties of the two-dimensional distribution of galaxy clusters.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..297d&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 4, p. 297 - 303

Astronomy and Astrophysics

Astrophysics

Clusters Of Galaxies: Distribution

Scientific paper

The authors investigate the fractal properties of the two-dimensional distribution of different richness and distance class subsamples for an all-sky catalog of rich clusters of galaxies. The results show that the two-dimensional distribution of the clusters can be described by a multi-level fractal structure. In the D ≤ 4 and D = 5+6 subsamples, the apparent turning scale between successive fractal levels is ≡42h-1Mpc. The fractal properties are similar in the northern and southern galactic latitudes on small and large scales.

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