A Numerical Study of Galaxy Properties from Cosmological Simulations with Star Formation

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dc.creatorYepes, G.
dc.creatorElizondo, D.
dc.creatorAscasibar, Y.
dc.date1999-05-31
dc.date.accessioned2026-07-07T02:31:46Z
dc.date.available2026-07-07T02:31:46Z
dc.descriptionFrom a set of 3D cosmological simulations which incorporate a self-consistent model of the star-gas interactions, we have been able to obtain a statistically significant sample of galaxy-type halos with observational properties, like colors and luminosities. Using this data-base, we have studied general relations of galaxies, such as the Tully-Fisher relation, luminosity functions, environmental dependences, or cosmic star formation density.
dc.description4 pages, 1 figure, to appear in proceedings of XIXth Moriond Astrophysics Meeting "Building galaxies: from the primordial universe to the present", March 13-20, 1999, Les Arcs, France
dc.identifierhttps://arxiv.org/abs/astro-ph/9905395
dc.identifierhttp://arxiv.org/abs/astro-ph/9905395
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14273
dc.subjectAstrophysics
dc.titleA Numerical Study of Galaxy Properties from Cosmological Simulations with Star Formation
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