Spectra of bulge stars with known abundance ratios for population synthesis

B. Barbuy, A. Alves-Brito, M. Zoccali, D. Minniti, V. Hill, A. Lecureur, A. Gómez, S. Ortolani, A. Renzini, P. Coelho, L. Sodré

Resultado de la investigación: Contribución a una revistaArtículo

Resumen

Spectra in the range 4000-7000 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.

Idioma originalInglés
Páginas (desde-hasta)87-90
Número de páginas4
PublicaciónProceedings of the International Astronomical Union
Volumen2
N.ºS241
DOI
EstadoPublicada - 1 dic 2006

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica

Huella Profundice en los temas de investigación de 'Spectra of bulge stars with known abundance ratios for population synthesis'. En conjunto forman una huella única.

  • Citar esto

    Barbuy, B., Alves-Brito, A., Zoccali, M., Minniti, D., Hill, V., Lecureur, A., Gómez, A., Ortolani, S., Renzini, A., Coelho, P., & Sodré, L. (2006). Spectra of bulge stars with known abundance ratios for population synthesis. Proceedings of the International Astronomical Union, 2(S241), 87-90. https://doi.org/10.1017/S1743921307007491