Morphological Evolution of Disc Galaxies in Chemodynamical Simulations

L. Michel-Dansac; H. Wozniak

doi:10.1051/eas:20070055

Issue		EAS Publications Series Volume 24, 2007 CRAL-2006. Chemodynamics: From First Stars to Local Galaxies


Page(s)		39 - 44
DOI		https://doi.org/10.1051/eas:20070055
Published online		21 April 2007

CRAL-2006. Chemodynamics: From First Stars to Local Galaxies
E. Emsellem, H. Wozniak, G. Massacrier, J.-F. Gonzalez, J. Devriendt and N. Champavert (eds)
EAS Publications Series, 24 (2007) 39-44

Morphological Evolution of Disc Galaxies in Chemodynamical Simulations

L. Michel-Dansac¹ and H. Wozniak²

¹ Instituto de Astronomía, UNAM, Ensenada, México
² Université de Lyon 1, CRAL, Lyon, France

Corresponding authors: This email address is being protected from spambots. You need JavaScript enabled to view it. ; This email address is being protected from spambots. You need JavaScript enabled to view it.

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.