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Chemodynamical models of barred galaxies

Published online by Cambridge University Press:  01 December 2006

Hervé Wozniak  and
Léo Michel-Dansac
Hervé Wozniak
Affiliation:
Université de Lyon 1, Centre de Recherche Astronomique de Lyon, Lyon, France email: [email protected]
Léo Michel-Dansac
Affiliation:
UNAM, Instituto de Astronomia, Ensenada, Mexico email: [email protected]
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Abstract

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Chemodynamical disc galaxy simulations calibrated with stellar populations synthesis models allow to build mock multi-wavelength images from numerical simulations. The morphological evolution of the mass and colour distributions can thus be simultaneously followed. We present the evolution of the stellar disc and bar structural parameters and summarize a number of important results we got in the recent past.

Keywords

galaxies: kinematics and dynamicsgalaxies: spiral
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 531 - 532
Copyright
Copyright © International Astronomical Union 2007

References

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Michel-Dansac, L. & Wozniak, H., 2007, in Chemodynamics: from the first stars to local galaxies, CRAL Conference Series I, held in Lyon 10-16 July 2007.Google Scholar
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Wozniak, H., & Michel–Dansac, L. 2007, in Chemodynamics: from the first stars to local galaxies, CRAL Conference Series I, held in Lyon 10-16 July 2007.Google Scholar
Wozniak, H., 2007 A&A acceptedGoogle Scholar