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Morphological Evolution of Disc Galaxiesin Chemodynamical Simulations

Published online by Cambridge University Press:  21 April 2007

E. Emsellem ,
H. Wozniak ,
G. Massacrier ,
J.-F. Gonzalez ,
J. Devriendt ,
N. Champavert ,
L. Michel-Dansac  and
H. Wozniak
L. Michel-Dansac*
Affiliation:
Instituto de Astronomía, UNAM, Ensenada, México
H. Wozniak
Affiliation:
Université de Lyon 1, CRAL, Lyon, France
*
[email protected] ; [email protected]
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Abstract

Chemodynamical disc galaxy simulations coupled with stellar populations synthesis models allow to build multi-wavelength images from numerical simulations, and then to follow their morphological evolution in colour and not only on the mass distribution. Using such technique, we present the evolution of several photometric observables, of the Tully-Fisher relation, as well as the evolution of disc structural parameters.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 24: CRAL-2006. Chemodynamics: From First Stars to Local Galaxies , 2007 , pp. 39 - 44
Copyright
© EAS, EDP Sciences, 2007

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