Statistical Properties of DLAs and sub-DLAs
| dc.creator | Peroux, Celine | |
| dc.creator | Irwin, Mike J. | |
| dc.creator | McMahon, Richard G. | |
| dc.creator | Storrie-Lombardi, Lisa J. | |
| dc.date | 2001-07-06 | |
| dc.date.accessioned | 2026-07-07T01:59:12Z | |
| dc.date.available | 2026-07-07T01:59:12Z | |
| dc.description | Quasar absorbers provide a powerful observational tool with which to probe both galaxies and the intergalactic medium up to high redshift. We present a study of the evolution of the column density distribution, f(N,z), and total neutral hydrogen mass in high-column density quasar absorbers using data from a recent high-redshift survey for damped Lyman-alpha (DLA) and Lyman limit system (LLS) absorbers. Whilst in the redshift range 2 to 3.5, ~90% of the neutral HI mass is in DLAs, we find that at z>3.5 this fraction drops to only 55% and that the remaining 'missing' mass fraction of the neutral gas lies in sub-DLAs with N(HI) 10^{19} - 2 * 10^{20} cm^{-2}. | |
| dc.description | 6 pages, 4 figures, in "Chemical Enrichment of Intracluster and Intergalactic medium", Proceedings of the Vulcano Workshop, May 14-18, 2001 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0107125 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0107125 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3019 | |
| dc.subject | Astrophysics | |
| dc.title | Statistical Properties of DLAs and sub-DLAs | |
| dc.type | text |