Comparisons of u-, g-, r-, i-, and z-band luminosity distributions between galaxy members of compact groups and isolated galaxies

Details Comparisons of u-, g-, r-, i-, and z-band luminosity distributions between galaxy members of compact groups and isolated galaxies Comparisons of u-, g-, r-, i-, and z-band luminosity distributions between galaxy members of compact groups and isolated galaxies

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011an....332..202d&link_type=abstract

Astronomische Nachrichten, Vol.332, Issue 2, p.202

Statistics

1

Galaxies: Fundamental Parameters, Galaxies: Statistics

Scientific paper

To investigate the environmental dependence of u-, g-, r-, i-, and z-band luminosities, we perform comparative studies of luminosity distributions between galaxy members of compact groups (CGs) and isolated galaxies. It is found that for the r, i, and z bands isolated galaxies have a higher proportion of faint galaxies and a lower proportion of luminous galaxies than galaxy members of CGs, but for the u band an opposite trend is observed. The correlation between the g-band luminosity and the environment has different trends in different luminosity regions.

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