Analysis of metallicity effects in SPH cosmological simulations

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dc.creatorTissera, P. B.
dc.creatorMosconi, A.
dc.creatorLambas, D. G.
dc.date1999-11-08
dc.date.accessioned2026-07-07T06:28:34Z
dc.date.available2026-07-07T06:28:34Z
dc.descriptionWe report preliminar results on a chemical model implemented in a hydrodynamical cosmological code. We compute the metallicity of the gaseous component in galactic halos at different redshifts. The results compare reasonably well to observations. In particular, we show the predicted metallicity content of today-galaxy progenitors as a function of redshift and confront them with those observed in DLA systems.
dc.description2 pages, 1 PS figures. To be published as an ASP Conference Series: Proceedings of Clustering at High Redshift, Les Rencontres Internationales de l'IGRAP
dc.identifierhttps://arxiv.org/abs/astro-ph/9911127
dc.identifierhttp://arxiv.org/abs/astro-ph/9911127
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97742
dc.subjectAstrophysics
dc.titleAnalysis of metallicity effects in SPH cosmological simulations
dc.typetext

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