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.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sucg.conf...47b&link_type=abstract

Workshop on Studying the Universe with Clusters of Galaxies, p. 47 - 51

Physics

Galaxy Distribution: Universe, Large-Scale Structure: Universe, Galaxy Clustering: Universe

Scientific paper

A statistical method based on the unnormalized integrated pair-counts of
objects is used to detect typical scales in various samples of galaxies
and clusters. For all samples there exists a scale of ≡60
h-1Mpc which can be interpreted as the typical scale of the
separation between superclusters, or the typical size of voids.

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