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Chemical evolution of disk galaxies in the local Universe using a new multiphase chemodynamical code
Published online by Cambridge University Press: 20 January 2011
Abstract
We aim to study of the formation and evolution of galaxies with high spatial and temporal resolution. We describe a new chemodynamical code to describe the physical interplay between the stars and the multiphase interstellar medium in galaxies, including a dust component. Preliminary results can be found in Champavert (2007).
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- Research Article
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- © EAS, EDP Sciences 2011