Making Damped Lyman Alpha Systems in Semi-Analytic Models

Details Making Damped Lyman Alpha Systems in Semi-Analytic Models Making Damped Lyman Alpha Systems in Semi-Analytic Models

1998-12-20

arxiv.org/abs/astro-ph/9812369v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, uses aipproc.sty, to appear in After the Dark Ages: The 9th Annual October Astrophysics Conference

Scientific paper

10.1063/1.58642

The velocity profiles of weak metal absorption lines can be used to observationally probe the kinematic state of gas in damped Lyman-alpha systems. Prochaska and Wolfe have argued that the flat distribution of velocity widths combined with the asymmetric line profiles indicate that the DLAS are disks with large rotation velocities. An alternative explanation has been proposed by Haehnelt, Steinmetz, and Rauch, in which the observed large velocity widths and asymmetric profiles can be produced by lines of sight passing through two or more clumps each having relatively small internal velocity dispersions. We investigate the plausibility of this scenario in the context of semi-analytic models based on hierarchical merging trees and including simple treatments of gas dynamics, star formation, supernova feedback, and chemical evolution. We find that all the observed properties of the metal-line systems including the distribution of velocities and the asymmetric profiles, can be reproduced by lines of sight passing through sub-clumps that are bound within larger virialized dark matter halos. In order to produce enough multiple hits, we find that the cold gas must be considerably more extended than the optical radius of the proto-galaxies, perhaps even beyond the tidal radius of the sub-halo. This could occur due to tidal stripping or supernova-driven outflows.

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