Numerical simulations of the intergalactic medium

Details Numerical simulations of the intergalactic medium Numerical simulations of the intergalactic medium

2002-09-05

arxiv.org/abs/astro-ph/0209094v1

Astronomy and Astrophysics

Astrophysics

Scientific paper

The intergalactic medium at redshifts 2--6 can be studied observationally through the absorption features it produces in the spectra of background quasars. Most of the UV-absorption lines arise in mildly overdense regions, which can be simulated reliably with current hydrodynamical simulations. Comparison of observed and simulated spectra allows one to put contraints on the model's parameters.

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