Collisional Ring Galaxies in Small Groups
Abstract
The probability of plunging orbits is enhanced in groups of galaxies and indeed, observations show that ring galaxies, which are believed to form when a galaxy passes through the center of a larger rotating disk, are often found in small groups. Numerical simulations combined with a knowledge of the large-scale HI distribution provide strong constraints on the dynamical history of these systems and on the identity of the intruder. Here we present a numerical model of the Cartwheel which supports the suggestion that the most distant companion is the intruder. We also present high-resolution HI observations of the more irregular system Arp 119 that reveal a possible connection to the most distant companion.
Cite
@article{arxiv.astro-ph/9910015,
title = {Collisional Ring Galaxies in Small Groups},
author = {Cathy Horellou},
journal= {arXiv preprint arXiv:astro-ph/9910015},
year = {2007}
}
Comments
4 pages, LaTex, 2 figures. To be published in ASP Conference Series, proceedings of the IAU Colloquium 174 on "Small Galaxy Groups" edited by M. Valtonen and C. Flynn