Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations

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...

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Hauptverfasser: Cora, S. A, Mosconi, M. B, Tissera, P. B, Lambas, D. G
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creator Cora, S. A
Mosconi, M. B
Tissera, P. B
Lambas, D. G
description 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.
doi_str_mv 10.48550/arxiv.astro-ph/0007072
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identifier DOI: 10.48550/arxiv.astro-ph/0007072
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subjects Physics - Astrophysics of Galaxies
Physics - Cosmology and Nongalactic Astrophysics
Physics - Earth and Planetary Astrophysics
Physics - High Energy Astrophysical Phenomena
Physics - Instrumentation and Methods for Astrophysics
Physics - Solar and Stellar Astrophysics
title Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations
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