Hostname: page-component-7c8c6479df-p566r Total loading time: 0 Render date: 2024-03-28T13:02:06.530Z Has data issue: false hasContentIssue false

Chemodynamical models of barred galaxies

Published online by Cambridge University Press:  01 December 2006

Hervé Wozniak
Affiliation:
Université de Lyon 1, Centre de Recherche Astronomique de Lyon, Lyon, France email: herve.wozniak@obs.univ-lyon1.fr
Léo Michel-Dansac
Affiliation:
UNAM, Instituto de Astronomia, Ensenada, Mexico email: leo@astrosen.unam.mx
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Bruzual, G., & Charlot, S., 1993, ApJ 405, 538CrossRefGoogle Scholar
Michel-Dansac&, L., & Wozniak, H., 2004, A&A 421, 863Google Scholar
Michel-Dansac, L., & Wozniak, H., 2006, A&A 452, 97Google Scholar
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
Kennicutt, R.C., 1998, ARA&A 36, 189Google Scholar
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