Red Galaxies from Hot Halos in Cosmological Hydro Simulations
Abstract
I highlight three results from cosmological hydrodynamic simulations that yield a realistic red sequence of galaxies: 1) Major galaxy mergers are not responsible for shutting off star-formation and forming the red sequence. Starvation in hot halos is. 2) Massive galaxies grow substantially (~ × 2 in mass) after being quenched, primarily via minor (1:5) mergers. 3) Hot halo quenching naturally explains why galaxies are red when they either (a) are massive or (b) live in dense environments.
- Publication:
-
The Intriguing Life of Massive Galaxies
- Pub Date:
- July 2013
- DOI:
- 10.1017/S1743921313005346
- arXiv:
- arXiv:1210.4943
- Bibcode:
- 2013IAUS..295..350G
- Keywords:
-
- galaxies: evolution;
- galaxies: interactions;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- 3 Figures, 4 pages. To appear in Proceedings of IAU Symposium No. 295: The intriguing life of massive galaxies