Star clusters as building blocks for dSph galaxies formation
Astrophysics of Galaxies
2015-05-14 v1 Cosmology and Nongalactic Astrophysics
Abstract
We study numerically the formation of dSph galaxies. Intense star bursts, e.g. in gas-rich environments, typically produce a few to a few hundred young star clusters, within a region of just a few hundred pc. The dynamical evolution of these star clusters may explain the formation of the luminous component of dwarf spheroidal galaxies (dSph). Here we perform a numerical experiment to show that the evolution of star clusters complexes in dark matter haloes can explain the formation of the luminous components of dSph galaxies.
Keywords
Cite
@article{arxiv.0910.0226,
title = {Star clusters as building blocks for dSph galaxies formation},
author = {P. Assmann and M. Fellhauer and M. I. Wilkinson},
journal= {arXiv preprint arXiv:0910.0226},
year = {2015}
}
Comments
4 pages, 4 figures, Proceedings of IAU symposium 266 'Star Clusters - Basic Building Blocks'