The Formation of Early-Type Galaxies: Observations to z=1
| dc.creator | Treu, T. | |
| dc.date | 2003-07-14 | |
| dc.date.accessioned | 2026-07-07T02:08:59Z | |
| dc.date.available | 2026-07-07T02:08:59Z | |
| dc.description | How does the number density of early-type galaxies (E+S0) evolve with redshift? What are their star formation histories? Do their mass density profile and other structural properties evolve with redshift? Answering these questions is key to understanding how E+S0s form and evolve. I review the observational evidence on these issues, focusing on the redshift range z=0.1-1, and compare it to the predictions of current models of galaxy formation. | |
| dc.description | 18 pages, 5 figures. Invited review to appear in "Carnegie Observatories Astrophysics Series, Vol. 3: Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution", ed. J. S. Mulchaey, A. Dressler, and A. Oemler (Cambridge: Cambridge Univ. Press) (submitted Apr 14 2003) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0307281 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0307281 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6275 | |
| dc.subject | Astrophysics | |
| dc.title | The Formation of Early-Type Galaxies: Observations to z=1 | |
| dc.type | text |