Elemental abundances at early times: the nature of Damped Lyman-alpha systems
| dc.creator | Molla, Mercedes | |
| dc.creator | Diaz, Angeles | |
| dc.creator | Ferrini, Federico | |
| dc.date | 1999-03-10 | |
| dc.date.accessioned | 2026-07-07T02:30:46Z | |
| dc.date.available | 2026-07-07T02:30:46Z | |
| dc.description | The distribution of element abundances with redshift in Damped Ly-alpha (DLA) systems can be adequately reproduced by the same model reproducing the halo and disk components of the Milky Way Galaxy at different galactocentric distances: DLA systems are well represented by normal spiral galaxies in their early evolutionary stages. | |
| dc.description | 2 pages, 1 figure, proceedings of X Rencontres de Blois, "The Birth of Galaxies" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9903150 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9903150 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13928 | |
| dc.subject | Astrophysics | |
| dc.title | Elemental abundances at early times: the nature of Damped Lyman-alpha systems | |
| dc.type | text |