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Dust in Nearby Groups of Galaxies?
Published online by Cambridge University Press: 08 February 2017
Abstract
The excess of higher redshift galaxies relative to the brightest member, found by several authors in poor, loose groups, is found to be present also in nearby, small groups identified by Geller and Huchra (1983) in the Center for Astrophysics Survey. This effect is explained as being due to the presence of diffuse intragroup dust together with an early evolutionary stage of nearby galaxy groups. An expected negative correlation between color excesses of galaxies and the velocity relative to the brightest member is found to be highly significant for both B-V and U-B colors. The optical depth produced by dust in groups turns out to be on the order of one, with a density of about 10−29 g/cm3.
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- IV. Extragalactic Background Radiation and Cosmology
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- Copyright © Kluwer 1990