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      The redshift evolution of Lyman-\(\alpha\) absorbers

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          Abstract

          We present a model for the Lyman-alpha absorbers that treats all objects (from the low-density forest clouds to the dense damped systems) in a unified description. This approach is consistent with an earlier model of galaxies (luminosity function, metallicity) but also with the known description of the density field in the small-scale non-linear regime. We consider two cosmological models: a critical universe \(\Omega=1\) with a CDM power-spectrum, and an open CDM universe with \(\Omega_0=0.3\), \(\Lambda=0\). We reproduce the available data on column density distribution as a function of redshift, the value of the main new parameter, the background ionizing UV flux, being consistent with the observed limits. This allows a quantitatively trustable analytical description of the opacity, mass, size, velocity dispersion and metallicity of these absorbers, over a range of column densities spanning 10 orders of magnitude. Moreover, together with an earlier model of galaxy formation this draws a unified picture of the redshift evolution of structures in the universe, from underdense clouds to massive high density galaxies, from weak to very deep potential wells.

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          Author and article information

          Journal
          25 March 1999
          astro-ph/9903388
          Custom metadata
          Astron.Astrophys. 345 (1999) 691
          23 pages, accepted for publication by A&A
          astro-ph

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