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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

H. Wozniak ,
G. Hensler ,
H. Wozniak ,
N. Champavert  and
H. Feldner
H. Wozniak
Affiliation:
Centre de Recherche Astrophysique de Lyon, 9 Av. Charles André, 69561 Saint-Genis-Laval Cedex, France
N. Champavert
Affiliation:
Centre de Recherche Astrophysique de Lyon, 9 Av. Charles André, 69561 Saint-Genis-Laval Cedex, France
H. Feldner
Affiliation:
Centre de Recherche Astrophysique de Lyon, 9 Av. Charles André, 69561 Saint-Genis-Laval Cedex, France
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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).

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 44: JENAM 2008: Grand Challenges in Computational Astrophysics , 2010 , pp. 41 - 42
Copyright
© EAS, EDP Sciences 2011

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References

Références

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