Small-scale substructure in relaxed clusters. I - Statistical characterization. II - Clustering model

Details Small-scale substructure in relaxed clusters. I - Statistical characterization. II - Clustering model Small-scale substructure in relaxed clusters. I - Statistical characterization. II - Clustering model

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410....1s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 410, no. 1, p. 1-20.

Statistics

Computation

43

Computational Astrophysics, Cosmology, Galactic Clusters, Statistical Analysis, Correlation Coefficients, Galactic Evolution

Scientific paper

The two-point correlation formalism is applied to the sample of galaxy clusters studied by Salvador-Sole et al. (1993) where evidence of correlation among galaxies was found. The two-point correlation that is obtained is used to derive the typical density profile of clumps in the frame of a realistic clustering model. The possible origin of clumps causing the correlation is discussed.

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