The second and third moments of Abell clusters and their three-point correlation function

Details The second and third moments of Abell clusters and their three-point correlation function The second and third moments of Abell clusters and their three-point correlation function

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cha%26a..14..102j&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 14, Issue 1, p. 102-111.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using the method of counts in cells we calculated the second and third moments in the angular distribution of northern Abell clusters with richness classes >= 1 and hence their spatial three-point correlation. We also calculated the three-point correlation function for a redshift sample of D<=4, R>=1 Abell clusters, the results are in agreement with those obtained for samples with estimated redshifts, thus showing further that the three-point correlation function of galaxies and Abell clusters can be described by a universal form.

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