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arxiv: astro-ph/0007072 · v1 · submitted 2000-07-06 · 🌌 astro-ph

Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations

S. A. Cora (Observatorio de La Plata , Argentia) , M. B. Mosconi (Observatorio de Cordoba , Argentina) , P. B. Tissera (Instituto de Astronomia y Fisica del Espacio , D. G. Lambas (Observatorio de Cordoba This is my paper
classification 🌌 astro-ph
keywords chemicalcosmologicalevolutionformationsimulationscluescodefirst
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We 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.

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