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Possible Existence of Dust in Nearby Galaxy Group

  • M. Girardi
  • G. Giuricin
  • F. Mardirossian
  • M. Mezzetti
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 165)

Abstract

The asymmetric distribution of galaxy redshifts in some nearby-group samples is explained as due to the existence of intragroup dust. The existence of a correlation between color excess of galaxies and radial velocity supports the hypothesis made.

Keywords

High Redshift Color Excess Galaxy Group Galaxy Redshift Redshift Distribution 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • M. Girardi
    • 1
  • G. Giuricin
    • 2
    • 3
  • F. Mardirossian
    • 2
    • 3
  • M. Mezzetti
    • 2
    • 3
  1. 1.International School for Advanced StudiesTriesteItaly
  2. 2.Department of AstronomyUniversity of TriesteTriesteItaly
  3. 3.C.I.R.A.CTriesteItaly

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