A generalized statistical criterion for the identification of optical and physical multiple systems, random and nonrandom groups of objects

Details A generalized statistical criterion for the identification of optical and physical multiple systems, random and nonrandom groups of objects A generalized statistical criterion for the identification of optical and physical multiple systems, random and nonrandom groups of objects

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..535a&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 535-548. In Russian.

Astronomy and Astrophysics

Astrophysics

17

Astrophysics, Galactic Clusters, Star Clusters, Statistical Analysis, Galactic Structure, Radial Velocity, Random Processes

Scientific paper

A statistical criterion has been proposed to reveal the random and physical clusterings among stars and galaxies. This criterion has been applied to nearby wide multiple stars, galaxy triplets and double galaxies where the primary components are the Seyfert galaxies. Confident and probable physical and optical systems have been discovered. The limit difference of radial velocities of components for the confident physical multiple galaxies has also been estimated.

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