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Spectra of bulge stars with known abundance ratios for population synthesis

Published online by Cambridge University Press:  01 December 2006

B. Barbuy
Affiliation:
IAG-USP, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected], [email protected]
A. Alves-Brito
Affiliation:
IAG-USP, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected], [email protected]
M. Zoccali
Affiliation:
PUC-Chile, Casilla 306, Santiago 22, Chile email: [email protected], [email protected]
D. Minniti
Affiliation:
PUC-Chile, Casilla 306, Santiago 22, Chile email: [email protected], [email protected]
V. Hill
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France email: [email protected], [email protected], [email protected]
A. Lecureur
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France email: [email protected], [email protected], [email protected]
A. Gómez
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon Cedex, France email: [email protected], [email protected], [email protected]
S. Ortolani
Affiliation:
Università di Padova, Dipartimento di Astronomia, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy, email: [email protected]
A. Renzini
Affiliation:
Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 2, I-35122 Padova, Italy email: [email protected]
P. Coelho
Affiliation:
IAG-USP, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected], [email protected]
L. Sodré
Affiliation:
IAG-USP, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected], [email protected]
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Abstract

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Spectra in the range 4000-7000 Å were obtained for a sample of bulge stars using the GMOS-Gemini low resolution spectrograph. The sample stars were selected from a VLT-FLAMES project for the observation of 1000 bulge stars, for which abundance ratios have been derived. Our aim is to study old stellar populations in external galaxies.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Bensby, T., Feltzing, S., & Lundström, I. 2004, A&A, 415, 155Google Scholar
Coelho, P., Barbuy, B., Perrin, M.-N., Idiart, T., Schiavon, R.P., Ortolani, S., & Bica, E. 2001, A&A, 376, 136Google Scholar
Lecureur, A., Zoccali, M., Hill, V., Barbuy, B., Goméz, A., Minniti, D., Ortolani, S., & Renzini, A. 2006, A&A, in press (astro-ph/10346)Google Scholar
Kormendy, J., & Kennicutt, R.C. 2004, ARA&A, 42, 603Google Scholar
Zoccali, M., Lecureur, A., Barbuy, B., Hill, V., Renzini, A., Minniti, D., Goméz, A., & Ortolani, S. 2006, A&A 457, L1Google Scholar