Small Groups of Galaxies: A Clue to a Critical Universe

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Abstract
We study the formation and the evolution of galaxy groups in a critical universe, showing the importance of secondary infall for their dynamical evolution. Merging is only slightly accelerated if galaxies have massive halos, because the mass initially associated to the individual galaxies is soon tidally stripped. Stripping is particularly effective for infalling galaxies, which thus avoid merging. We find that, as a rule, merging is effectively terminated when infall becomes dominant. We look for compact groups in our ensemble of simulations, and compare their statistical properties with Hickson's compact groups. We then discuss in terms of the Press & Schechter formalism the statistics of such groups and their evolution in different cosmological scenarios. We show that compact group formation is an ongoing and frequent process in a critical universe. Our model reconciles the contradiction between the observed absence of young merger remnants and the high rate of galaxy interactions expected in compact groups. In open universes, instead, earlier formation of groups and suppression of secondary infall makes it more unlikely that compact groups survive as such until the present. We conclude that the existence of dense and dynamically young groups of galaxies like HCGs points towards a high-density universe.
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