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A Classification of the Galaxy Groups

Published online by Cambridge University Press:  12 April 2016

Joanna P. Anosova*
Affiliation:
Astronomical Observatory Leningrad State University, Bibliotechnaya p1.1 198904 Leningrad Petrodvorets, USSR

Abstract

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A statistical criterion has been proposed to reveal the random and physical clusterings among stars, galaxies and other objects. This criterion has been applied to the galaxy triples of the list by Karachentseva, Karaschentsev and Scherbanovsky, and the double galaxies of the list by Dahari where the primary components are the Seyfert galaxies. The confident physical, probable physical, probable optical and confident optical groups have been identified. The limit difference of radial velocities of components for the confident physical multiple galaxies has also been estimated.

Type
VIII. Classical Theory of Multiplets
Copyright
Copyright © NASA 1990

References

Anosova, J.P. 1986, Astrofizika, 25, 2 297.Google Scholar
Anosova, J. P. 1987, Astrofizika, 27, 3 535.Google Scholar
Anosova, J. P. 1988, Astrophys. Space Sci., 142, 12, 103.Google Scholar
Dahari, O. 1985, Astron. J., 90, 1772.CrossRefGoogle Scholar
Karachentseva, V. E., Karachentsev, I. D., Sherbanovsky, A. L. 1979, Izv. Spec. Astrofiz. Obs., 11 3.Google Scholar
Meterne, J. 1978, Astron. Astrophys., 63 401.Google Scholar