Cluster Ellipticals at High Redshift: The View from the Ground and with HST
Abstract
New ground-based and HST observations of distant clusters make it possible to trace the history of E/S0 galaxies to lookback times of ~10 Gyr. The data strongly favor a scenario in which cluster ellipticals formed very early with a narrow spread in ages. By z = 1.2 there are changes in color and luminosity consistent with simple passive evolution, but even at that redshift the galaxies appear mature, with red colors suggesting ages of several Gyr. Apparently we are still falling well short of seeing the true epoch of formation.
Keywords
Cite
@article{arxiv.astro-ph/9507064,
title = {Cluster Ellipticals at High Redshift: The View from the Ground and with HST},
author = {Mark Dickinson},
journal= {arXiv preprint arXiv:astro-ph/9507064},
year = {2007}
}
Comments
10 page postscript file including 6 figures, uuencoded, gzip-compressed, self-unpacking, and so forth. To appear in "Fresh Views on Elliptical Galaxies," proceedings of a conference held in Puebla, Mexico, 14-17 March 1995