Clustering of near clusters versus cluster compactness

Details Clustering of near clusters versus cluster compactness Clustering of near clusters versus cluster compactness

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..559g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Feb. 1, 1989, p. 559-565.

Astronomy and Astrophysics

Astronomy

1

Astrometry, Galactic Clusters, Universe, Angular Correlation, Cosmology, Mass Distribution, Open Clusters, Spatial Distribution

Scientific paper

The clustering properties of near Zwicky clusters are studied by using the two-point angular correlation function. The angular correlation functions for compact and medium compact clusters, for open clusters, and for all near Zwicky clusters are estimated. The results show much stronger clustering for compact and medium compact clusters than for open clusters, and that open clusters have nearly the same clustering strength as galaxies.

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