Two-point correlation for rich clusters of galaxies

Details Two-point correlation for rich clusters of galaxies Two-point correlation for rich clusters of galaxies

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvl..56.1878o&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 56, April 28, 1986, p. 1878-1881.

Astronomy and Astrophysics

Astronomy

14

Correlation, Cosmology, Galactic Clusters, Galactic Evolution, Astronomical Models, Mass Distribution, Power Spectra

Scientific paper

The rich-cluster two-point correlation function is examined in a model
where rich clusters of galaxies form at high peaks of primordial
Gaussian mass-density fluctuations (averaged over a suitable volume).
Particular attention is paid to the case when the primordial
fluctuations have a Zel'dovich power spectrum.

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