Surface Brightness Evolution of Cluster Galaxies
| dc.creator | Schade, David | |
| dc.date | 1996-12-17 | |
| dc.date.accessioned | 2026-07-07T02:22:35Z | |
| dc.date.available | 2026-07-07T02:22:35Z | |
| dc.description | Surface brightness evolution has been detected in elliptical galaxies (consistent with passive evolution models of old stellar populations) and in disk galaxies (presumably due to enhanced star-formation rates). The rates of evolution in clusters and the field are not measurably different. In addition to this similarity, the high-redshift populations in both environments exhibit a ``blue-excess'' population, increased rates of star formation, and high frequency of peculiar structure. Thus, there are several parallels between evolving cluster and field galaxies and the high-redshift cluster environment will be understood only by comparison with the field population at the same epoch. | |
| dc.description | To appear in proceeding of the 37th Herstmonceux conference: HST and the High Redshift Universe | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9612170 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9612170 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10929 | |
| dc.subject | Astrophysics | |
| dc.title | Surface Brightness Evolution of Cluster Galaxies | |
| dc.type | text |