Damped Lyman-alpha and Lyman Limit Absorbers in the Cold Dark Matter Model

Details Damped Lyman-alpha and Lyman Limit Absorbers in the Cold Dark Matter Model Damped Lyman-alpha and Lyman Limit Absorbers in the Cold Dark Matter Model

1995-09-21

arxiv.org/abs/astro-ph/9509106v1

Astrophys.J. 457 (1996) L57

Astronomy and Astrophysics

Astrophysics

compressed postscript, 12 pages including 2 embedded figures. A version that also includes embedded Figure 1, a 6 Mbyte color

Scientific paper

10.1086/309900

We study the formation of damped \lya and Lyman limit absorbers in a hierarchical clustering scenario using a gas dynamical simulation of an $\Omega = 1$, cold dark matter universe. In the simulation, these high column density systems are associated with forming galaxies. Damped \lya absorption, $N_{HI} \simgt 10^{20.2}\cm^{-2}$, arises along lines of sight that pass near the centers of relatively massive, dense protogalaxies. Lyman limit absorption, $10^{17}\cm^{-2} \simlt N_{HI} \simlt 10^{20.2}\cm^{-2}$, develops on lines of sight that pass through the outer parts of such objects or near the centers of smaller protogalaxies. The number of Lyman limit systems is less than observed, while the number of damped \lya systems is quite close to the observed abundance. Damped absorbers are typically $\sim 10$ kpc in radius, but the population has a large total cross section because the systems are much more numerous than present day $L_*$ galaxies. Our results demonstrate that high column density systems like those observed arise naturally in a hierarchical theory of galaxy formation and that it is now possible to study these absorbers directly from numerical simulations.

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