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 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acasn..30..241j&link_type=abstract

(Acta Astronomica Sinica, vol. 30, no. 3, 1989, p. 241-248) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, March

Astronomy and Astrophysics

Astrophysics

Galactic Clusters, Galactic Structure, Statistical Correlation, Angular Distribution, Northern Sky, Red Shift, Spatial Distribution

Scientific paper

The method of counts in cells was used to calculate the second and third moments in the angular distribution of northern Abell clusters with richness classes equal to or greater than 1 and hence their spatial three-point correlation. The three-point correlation function was also calculated for a redshift sample of 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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