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
Instituto de Astronomía, UNAM,
2 Université de Lyon 1, CRAL, Lyon, France
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.
© EAS, EDP Sciences, 2007