Simulating Gas at High Redshift

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dc.creatorKatz, Neal
dc.creatorHernquist, Lars
dc.creatorWeinberg, David H.
dc.date1998-01-09
dc.date.accessioned2026-07-07T02:25:46Z
dc.date.available2026-07-07T02:25:46Z
dc.descriptionWe discuss simulations of gas at high redshift. We briefly review the methods used and the results for quasar absorption lines. We present gas mass functions and galaxy correlation functions for 5 different cosmological models. Galaxies should be detectable at redshifts greater than 2 by SKAI, and measurements of the gas mass functions and galaxy correlation functions could be used to discriminate between different cosmological models.
dc.description9 pages, 4 figures in text, LaTex (paspconf.sty) To appear in the conference proceedings of Highly Redshifted Radio Lines
dc.identifierhttps://arxiv.org/abs/astro-ph/9801074
dc.identifierhttp://arxiv.org/abs/astro-ph/9801074
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12003
dc.subjectAstrophysics
dc.titleSimulating Gas at High Redshift
dc.typetext

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