Evolution of the Red Sequence in simulated galaxy groups
Astrophysics
2007-05-23 v1
Abstract
N--body + hydrodynamical simulations of formation and evolution of galaxy groups in a LambdaCDM cosmology have been performed. The properties of the galaxy populations in 12 groups are here discussed, with focus on the colour-magnitude relation in both normal and fossil groups.
Cite
@article{arxiv.astro-ph/0612423,
title = {Evolution of the Red Sequence in simulated galaxy groups},
author = {A. D. Romeo and N. R. Napolitano and G. Covone and J. Sommer-Larsen},
journal= {arXiv preprint arXiv:astro-ph/0612423},
year = {2007}
}
Comments
Proceedings of the Conference "DEEP06 - At the edge of the Universe", Sintra, 9-13 October 2006; 5 pages, 3 colour figures