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A New Chemo-Dynamical Tool to Study The Evolution of Galaxies in the Local Universe

Published online by Cambridge University Press:  01 August 2006

Nicolas Champavert  and
Hervé Wozniak
Nicolas Champavert
Affiliation:
Centre de Recherche Astronomique de Lyon, France; email: champavert@obs.univ-lyon1.fr
Hervé Wozniak
Affiliation:
Centre de Recherche Astronomique de Lyon, France; email: champavert@obs.univ-lyon1.fr
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Abstract

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Figure 1.

Schematic presentation of our new chemo-dynamical tool. See Champavert & Wozniak (2007a) for full details and references.

Keywords

galaxies: evolutionISM: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 306
Copyright
Copyright © International Astronomical Union 2007

References

Champavert, N. & Wozniak, H. 2007a, in: Chemodynamics: from first stars to local galaxies, CRAL Conference Series I, Emsellem et al. (eds), in press.Google Scholar
Champavert, N. & Wozniak, H. 2007b, in: Heating vs. Cooling in Galaxies and Clusters of Galaxies, ESO Astrophysics Symposia Series, Garching, Boehringer et al. (eds), in press.Google Scholar