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The Magellanic Clouds Chemical Enrichment History via Ca II Triplet Spectroscopy

Published online by Cambridge University Press:  01 December 2006

R. Carrera ,
C. Gallart ,
A. Aparicio ,
E. Costa ,
E. Hardy ,
R. Méndez  and
N. Noël
R. Carrera
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain email: [email protected]
C. Gallart
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain email: [email protected]
A. Aparicio
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain email: [email protected] Departamento de Astrofísica, Universidad de La Laguna, Spain
E. Costa
Affiliation:
Departamento de Astronomía, Universidad de Chile, Chile
E. Hardy
Affiliation:
National Radio Astronomy Observatory, Chile
R. Méndez
Affiliation:
Departamento de Astronomía, Universidad de Chile, Chile
N. Noël
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain email: [email protected]
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Abstract

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We report the results of our project devoted to study the chemical enrichment history of the field population in the Magellanic Clouds using Ca II triplet spectroscopy.

Keywords

galaxies: abundancesgalaxies: individual (LMC SMC)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 323 - 324
Copyright
Copyright © International Astronomical Union 2007

References

Carrera, R. 2006, PhD thesis, Uniersidad de la Laguna, SpainGoogle Scholar
Carrera, R., Gallart, C., Pancino, E., & Zinn, R. 2007, AJ, SubmittedGoogle Scholar
Cole, A. A. et al. , 2005, AJ, 129, 1465Google Scholar
Dirsch, B. et al. 2000, A&A, 360, 133Google Scholar
Dopita, M. A. et al. 1997, ApJ, 474, 188Google Scholar