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Metal-poor globular clusters of the galactic bulge

Published online by Cambridge University Press:  09 March 2010

B. Barbuy
Affiliation:
Universidade de São Paulo, Brazil
S. Ortolani
Affiliation:
Università di Padova, Italy
M. Zoccali
Affiliation:
Pontificia Universidad Catolica de Chile, Chile
V. Hill
Affiliation:
Observatoire de la Côte d'Azur, France
D. Minniti
Affiliation:
Pontificia Universidad Catolica de Chile, Chile
E. Bica
Affiliation:
Universidade Federal do Rio Grande do Sul, Brazil
A. Renzini
Affiliation:
Osservatorio Astronomico di Padova, Italy
A. Gómez
Affiliation:
Observatoire de Paris-Meudon, France
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Abstract

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Very few abundance analyses of individual stars in metal-poor globular clusters in the galactic bulge are available. The main purpose of this study is to derive abundances in individual stars of such clusters, in order to establish their abundance pattern, trying to characterize the oldest bulge stellar populations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

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