The star-forming progenitors of massive red galaxies
Abstract
The link between massive red galaxies in the local Universe and star-forming galaxies at high redshift is investigated with a semi-analytic model that has proven successful in many ways, e.g. explaining the galaxy colour-magnitude bimodality and the stellar mass-age relation for red-sequence galaxies. The model is used to explore the processes that drive star formation in different types of galaxies as a function of stellar mass and redshift. We find that most z=2-4 star-forming galaxies with M_*>10^10 M_Sun evolve into red-sequence galaxies. Also, most of the massive galaxies on the red-sequence today have passed through a phase of intense star formation at z>2. Specifically, ~ 90% of today's red galaxies with M_*>10^11 M_Sun were fed during this phase by cold streams including minor mergers. Gas-rich major mergers are rare and the effects of merger-driven starbursts are ephemeral. On the other hand, major mergers are important in powering the most extreme starbursts. Gas-rich mergers also explain the tail of intermediate-mass red galaxies that form relatively late, after the epoch of peak star formation. In two thirds of the currently red galaxies that had an intense star formation event at , this event was triggered by a merger.
Keywords
Cite
@article{arxiv.1301.2067,
title = {The star-forming progenitors of massive red galaxies},
author = {Andrea Cattaneo and Joanna Woo and Avishai Dekel and Sandra M. Faber},
journal= {arXiv preprint arXiv:1301.2067},
year = {2015}
}
Comments
15 pages, 11 figures, accepted for publication on MNRAS