Peculiarities of binary galaxies

Computer Science

Scientific paper

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Galactic Radiation, Galactic Structure, Galactic Evolution, Luminous Intensity

Scientific paper

A statistical assumption relating the true separation of two galaxies within a binary to their projected rectilinear separation is evaluated, and a possible explanation for the greater luminosity of binary galaxies compared to field galaxies is discussed. The distribution of the angle relating the true to the projected separation is analyzed by a test analogous to the V/Vmax test for quasars which considers the angular separation of the galaxies and the maximum separation that the pair could have had and still be included in the sample for a sample of 156 pairs of galaxies. Results support the argument of White and Valdes (in press) based on the orientation distribution of pairs isolated from an uncorrelated population. An examination of the colors of binary galaxies suggests that color changes due to increased star formation caused by galactic interaction are capable of accounting for the one-magnitude increase in B magnitude observed in binary galaxies.

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