Development of the Red Sequence in Galaxy Clusters
Cosmology and Nongalactic Astrophysics
2020-04-15 v1
Abstract
We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by using a combination of a cosmological N-body simulation of a cluster of galaxies and a semi-analytic model of galaxy formation. The departure of galaxies in the bright end of the CMR with respect to the trend defined by less luminous galaxies could be explained by the influence of minor mergers.
Cite
@article{arxiv.1107.0974,
title = {Development of the Red Sequence in Galaxy Clusters},
author = {Noelia Jiménez and Sofía A. Cora and Analía Smith Castelli and Lilia P. Bassino},
journal= {arXiv preprint arXiv:1107.0974},
year = {2020}
}
Comments
Proceedings IAU Symposium No. 267, 2009. Co-Evolution of Central Black Holes and Galaxies