Galaxy Formation and Chemical Evolution in Hierarchical Hydrodynamical Simulations
arXiv:astro-ph/0007072
Abstract
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.
4 pages, 1 Postscript figure, 1jpg figure. To appear in ASP, Conference Series. Proceeding of 'Stars, Gas and Dust in Galaxies: Exploring the Links'