Galaxy and star formation up to z ~ 1
| dc.creator | Hammer, F. | |
| dc.creator | Flores, H. | |
| dc.date | 2001-09-21 | |
| dc.date.accessioned | 2026-07-07T02:00:11Z | |
| dc.date.available | 2026-07-07T02:00:11Z | |
| dc.description | Star formation history shows a gradual decline since the last 8-9 Gyr (z=1). The bulk of present-day stellar mass and metal content was formed at redshifts lower than 2-3, which is consistent with a hierarchical scenario of galaxy formation. Observations of galaxy evolution during the last 2/3 of the Universe age could be done in great details, and provide numerous insights on the origin of the Hubble diagram. To some extent, the evolution and formation of present-day elliptical and spiral galaxies could be related to the most rapidly evolving galaxy populations at z ~ 1, namely the luminous IR galaxies and the luminous compact galaxies. | |
| dc.description | SF2A Proceedings 28 Mai - 1er Juin 2001, Lyon, 7 pages and 2 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0109384 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0109384 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3371 | |
| dc.subject | Astrophysics | |
| dc.title | Galaxy and star formation up to z ~ 1 | |
| dc.type | text |