The Epochs of Early‐Type Galaxy Formation as a Function of Environment
Max Planck Institute for Extraterrestrial Physics · Stuttgart Observatory · +1 more institution
Abstract
The aim of this paper is to set constraints of the epochs of early-type galaxy formation through the 'archaeology' of the stellar populations in local galaxies. Using our models of absorption line indices that account for variable abundance ratios, we derive the stellar population parameters of 124 early-type galaxies in high and low density environments. We find that all three parameters age, metallicity, and alpha/Fe ratio are correlated with velocity dispersion. We further find evidence for an influence of the environment on the stellar population properties. Massive early-type galaxies in low-density environments appear on average ~2 Gyrs younger and slightly more metal-rich than their counterparts in high…
Citation impact
- FWCI
- 61.79
- Percentile
- 100%
- References
- 203
Authors
4- DTD. ThomasCorresponding
Max Planck Institute for Extraterrestrial Physics, Stuttgart Observatory
- CMClaudia Maraston
Stuttgart Observatory, Max Planck Institute for Extraterrestrial Physics
- RBR. Bender
Stuttgart Observatory, Max Planck Institute for Extraterrestrial Physics
- CMC. Mendes de Oliveira
Universidade de São Paulo
Topics & keywords
- Astrophysics
- Physics
- Galaxy
- Metallicity
- Velocity dispersion
- Stellar mass
- Galaxy formation and evolution
- Monte Carlo method