Numerical simulations of the intergalactic medium

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dc.creatorTheuns, Tom
dc.date2002-09-05
dc.date.accessioned2026-07-07T02:04:59Z
dc.date.available2026-07-07T02:04:59Z
dc.descriptionThe 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.
dc.identifierhttps://arxiv.org/abs/astro-ph/0209094
dc.identifierhttp://arxiv.org/abs/astro-ph/0209094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4971
dc.subjectAstrophysics
dc.titleNumerical simulations of the intergalactic medium
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