The Luminosity Function of Galaxies in Compact Groups

Abstract

From R-band images of 39 Hickson compact groups (HCGs), we use galaxy counts to determine a luminosity function extending to M_R=-14.0, approximately two magnitudes deeper than previous compact group luminosity functions. We find that a single Schechter function is a poor fit to the data, so we fit a composite function consisting of separate Schechter functions for the bright and faint galaxies. The bright end is best fit with M^*=-21.6 and alpha=-0.52 and the faint end with M^*=-16.1 and alpha=-1.17. The decreasing bright end slope implies a deficit of intermediate luminosity galaxies in our sample of HCGs and the faint end slope is slightly steeper than that reported for earlier HCG luminosity functions. Furthermore, luminosity functions of subsets of our sample reveal more substantial dwarf populations for groups with x-ray halos, groups with tidal dwarf candidates, and groups with a dominant elliptical or lenticular galaxy. Collectively, these results support the hypothesis that within compact groups, the initial dwarf galaxy population is replenished by "subsequent generations" formed in the tidal debris of giant galaxy interactions.

26 pages, to be published in The Astrophysical Journal, 8 greyscale plates (figures 1 and 2) can be retrieved at http://www.astro.psu.edu/users/sdh/pubs.html

References in corpus (6)

• The Properties of Poor Groups of Galaxies: I. Spectroscopic Survey and Results
• The Properties of Poor Groups of Galaxies: II. X-ray and Optical Comparisons
• Dwarf Galaxies in the Coma Cluster. II. Photometry and Analysis
• The dwarf galaxy population of the Coma cluster to M_R=-11
• The local space density of dwarf galaxies
• The Durham/UKST Galaxy Redshift Survey - II. The Field Galaxy Luminosity Function

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• The Beginning of the End: Hubble Space Telescope Images of Seyfert's Sextet
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