Spectra of bulge stars with known abundance ratios for population synthesis
Abstract
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. © 2007 International Astronomical Union.
Más información
| Título de la Revista: | Proceedings of the International Astronomical Union |
| Volumen: | 2 |
| Número: | S241 |
| Editorial: | Cambridge University Press |
| Fecha de publicación: | 2006 |
| Página de inicio: | 87 |
| Página final: | 90 |
| URL: | http://www.scopus.com/inward/record.url?eid=2-s2.0-37149011956&partnerID=q2rCbXpz |