Correlation functions for pairs and groups of galaxies

Details Correlation functions for pairs and groups of galaxies Correlation functions for pairs and groups of galaxies

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3098..149k&link_type=abstract

In NASA, Marshall Space Flight Center, Paired and Interacting Galaxies: International Astronomical Union Colloquium No. 124 p 14

Astronomy and Astrophysics

Astronomy

2

Correlation, Distance, Galactic Clusters, Galaxies, Red Shift, Astronomy, Spatial Distribution

Scientific paper

There are many studies on the correlation functions of galaxies, of clusters of galaxies, even of superclusters (e.g., Groth and Peebles 1977; Davies and Peebles 1983; Kalinkov and Kuneva 1985, 1986; Bahcall 1988 and references therein) but not so many on pairs and groups of galaxies. Results of the calculations of two-point correlation fuctions for some catalogs of pairs and groups of galaxies are given. It is assumed that the distances to pairs and groups of galaxies are given by their mean redshifts according to R = sigma ni-1 Vi/nH0, where n is the number of galaxies in the system and H0 = 100 km s-1 Mpc-1.

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