Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations

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dc.creatorCora, S. A.
dc.creatorMosconi, M. B.
dc.creatorTissera, P. B.
dc.creatorLambas, D. G.
dc.date2000-07-06
dc.date.accessioned2026-07-07T01:54:17Z
dc.date.available2026-07-07T01:54:17Z
dc.descriptionWe report first results of an implementation of a chemical model in a cosmological code, based on the Smoothed Particle Hydrodynamics (SPH) technique. We show that chemical SPH simulations are a promising tool to provide clues for the understanding of the chemical properties of galaxies in relation to their formation and evolution in a cosmological framework.
dc.description4 pages, 1 Postscript figure, 1jpg figure. To appear in ASP, Conference Series. Proceeding of 'Stars, Gas and Dust in Galaxies: Exploring the Links'
dc.identifierhttps://arxiv.org/abs/astro-ph/0007072
dc.identifierhttp://arxiv.org/abs/astro-ph/0007072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1285
dc.subjectAstrophysics
dc.titleGalaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations
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