paper

Very deep spectroscopy of the Coma cluster line of sight: exploring new territories

arXiv:0906.4443 · doi:10.1051/0004-6361/200912228

Abstract

Environmental effects have an important influence on cluster galaxies, but studies at very faint magnitudes (R>21) are almost exclusively based on imaging. We present here a very deep spectroscopic survey of galaxies on the line of sight to Coma, based on redshifts obtained with VLT/VIMOS for 715 galaxies in the unprecedented magnitude range 21<R<23 (absolute magnitude -14 to -12). We confirm the substructures previously identified in Coma by Adami et al. (2005a), and identify three new ones. We detect many groups behind Coma: a large structure at z~0.5, the SDSS Great Wall, and a large and very young structure at z~0.054. These structures account for the mass maps derived from a recent weak lensing analysis by Gavazzi et al. (2009). The orbits of dwarf galaxies are probably anisotropic and radial, and could originate from field galaxies radially falling into the cluster. Spectral characteristics of Coma dwarf galaxies show that red or absorption line galaxies have larger stellar masses and are older than blue or emission line galaxies. R<22 galaxies show less prominent absorption lines than R>22 galaxies. This trend is less clear for field galaxies, suggesting that part of the faint Coma galaxies could have been recently injected from the field following the NGC 4911 group infall. We present a list of five Ultra Compact Dwarf galaxy candidates. We also globally confirm spectroscopically our previous results on the galaxy luminosity functions and find that dwarf galaxies follow a red sequence similar to that drawn by bright galaxies. Dwarf galaxies are very abundant in Coma, and are partly field galaxies that have fallen onto the cluster along filaments.

Accepted for publication in Astronomy & Astrophysics

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