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Stellar abundances tracing the formation of the Galactic Bulge

Published online by Cambridge University Press:  01 June 2008

Beatriz Barbuy ,
Manuela Zoccali ,
Sergio Ortolani ,
Vanessa Hill ,
Alvio Renzini ,
Jorge Meléndez ,
Anita Gómez ,
Martin Asplund ,
Dante Minniti  and
Eduardo Bica
...Show all authors
Beatriz Barbuy
Affiliation:
Universidade de São Paulo, IAG, Rua do Matão 1226São Paulo 05508-900, Brazil email: [email protected]
Manuela Zoccali
Affiliation:
Universidad Catolica de Chile, Department of Astronomy & Astrophysics, Casilla 306, Santiago 22, Chile email: [email protected], [email protected]
Sergio Ortolani
Affiliation:
Università di Padova, Dipartimento di Astronomia, Vicolo dell'Osservatorio 2, I-35122 Padova, Italy email: [email protected]
Vanessa Hill
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France email: [email protected], [email protected]
Alvio Renzini
Affiliation:
Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy email: [email protected]
Jorge Meléndez
Affiliation:
Centro de Astrofísica da Universidade de Porto, Rua das Estrelas, 4150-762 Porto, Portugal email: [email protected]
Anita Gómez
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France email: [email protected], [email protected]
Martin Asplund
Affiliation:
Max Planck Institute for Astrophysics, Postfach 1317, 85741 Garching, Germany email: [email protected]
Dante Minniti
Affiliation:
Universidad Catolica de Chile, Department of Astronomy & Astrophysics, Casilla 306, Santiago 22, Chile email: [email protected], [email protected]
Eduardo Bica
Affiliation:
Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, Porto Alegre 91501-970, Brazil e-mail: [email protected]
Alan Alves-Brito
Affiliation:
Universidade de São Paulo, IAG, Rua do Matão 1226São Paulo 05508-900, Brazil email: [email protected]
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Abstract

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The metallicity distribution and abundance ratios of the Galactic bulge are reviewed. Issues raised by different groups in recent work, in particular the high metallicity end, a comparison between the oxygen abundances derived from different indicators, the [OI] 630nm and IR OH lines, and the issue of measuring giants vs. dwarfs, are discussed. Finally, abundances in bulge globular clusters are briefly described.

Keywords

Galaxy: abundancesbulgestellar contentglobular clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Issue S254: The Galaxy Disk in Cosmological Context , June 2008 , pp. 153 - 158
Copyright
Copyright © International Astronomical Union 2009

References

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