Satellite galaxies in nearby groups of galaxies
arXiv:1512.04838
Abstract
We analyse distribution, kinematics and star-formation (SF) properties of satellite galaxies in three different samples of nearby groups. We find that studied groups are generally well approximated by low-concentration NFW model, show a variety of LOS velocity dispersion profiles and signs of SF quenching in outskirts of dwarf satellite galaxies.
5 pages, 2 figures, poster paper presented at the workshop "Let's group - The life cycle of galaxies in their favorite environment", held in 16-19 June 2015 at ESO Headquarter, Garching, Germany