English

The Galaxy Group/Cosmology Connections

Astrophysics 2007-05-23 v1

Abstract

\def\spose#1{\hbox to 0pt{#1\hss}} \def\lta{\mathrel{\spose{\lower 3pt\hbox{\mathchar"218\mathchar"218}} \raise 2.0pt\hbox{\mathchar"13C\mathchar"13C}}} Groups of galaxies are highly linked to cosmology: 1) groups are tidally destroyed by the tidal field of the cluster they fall into; 2) spherical infall leads to the young cosmo-dynamical state of loose groups, a fundamental surface for groups, Ω00.3\Omega_0 \simeq 0.3, and the mixed nature of compact groups (virialized groups, groups at full collapse, and chance alignments within collapsing loose groups, for decreasing compact group velocity dispersion) ; 3) X-ray analyses lead to Ω0\lta0.5\Omega_0 \lta 0.5.

Keywords

Cite

@article{arxiv.astro-ph/9406043,
  title  = {The Galaxy Group/Cosmology Connections},
  author = {Gary A. Mamon},
  journal= {arXiv preprint arXiv:astro-ph/9406043},
  year   = {2007}
}

Comments

6 pages (2 figures included), uuencoded tared postscript file, to appear in XIVth Moriond Astrophysics Meeting "Clusters of Galaxies", ed. F. Durret, A. Mazure, S.D.M. White & J. Tran Thanh Van (Gif-sur-Yvette: Eds. Fronti\`eres), in press, IAP preprint 461

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