Typical Scales in the Distribution of Galaxies and Clusters

Details Typical Scales in the Distribution of Galaxies and Clusters Typical Scales in the Distribution of Galaxies and Clusters

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.7104b&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #71.04; Bulletin of the American Astronomical Society, Vol. 25, p.1399

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Scientific paper

A systematic analysis of available catalogues of optical ,infrared galaxies,pencil beams and clusters of galaxies has been carried out.the statistical method is based on detecting changes in the unnormalized pair counts. It is very effective in discovering coherent structures. In all data samples a characteristic scale of 60(h-1)mpc was found. In deep samples an additional large scale of 130mpc is detected. The 60mpc scale might be the typical distance between superclusters, or in other words the characteristic scale of voids.

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