Abstract
We describe observations focused on understanding the epochs and timescales of the formation and evolution of early-type galaxies, particularly those in clusters. We show that while early-type cluster galaxies are on average older and closer to coeval than their counterparts in the field, significant age spreads (a factor of two in massive ellipticals, more in low-mass galaxies, especially S0’s) still exist in these objects. We then show that it is now possible to detect the evolution of early-type galaxies directly by comparing deep absorption-line spectroscopy of intermediate-redshift cluster galaxies with local cluster galaxies. We find that the stellar populations of early-type cluster galaxies do indeed evolve, at a rate that appears to be consistent with the cosmological lookback time.
Preview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Editor information
Rights and permissions
About this paper
Cite this paper
Trager, S., Faber, S., Dressler, A. Directly Detecting the Evolution of Early-Type Galaxies. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_35
Download citation
DOI: https://doi.org/10.1007/10995020_35
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)