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Typical Characteristics of Chance and Non-Chance Compact Groups of Galaxies
Published online by Cambridge University Press: 25 May 2016
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In our previous works (Anosova 1987, Anosova and Kiseleva 1993) we developed a new objective statistical method for an identification of members of star and galaxy clusters as chance or non-chance ones. In the case of galaxies this method uses simultaneously their radial velocities V and angular separations ρ.
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- Part II: Contributed Papers
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- Copyright © Kluwer 1996
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