Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-22T16:50:50.761Z Has data issue: false hasContentIssue false

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
Affiliation:
Centre de Recherche Astronomique de Lyon, France; email: [email protected]
Hervé Wozniak
Affiliation:
Centre de Recherche Astronomique de Lyon, France; email: [email protected]
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.

Figure 1.

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

Type
Contributed Papers
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