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: Article

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

Huella dactilar

stars
synthesis
spectrographs
galaxies
project

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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. / Spectra of bulge stars with known abundance ratios for population synthesis. En: Proceedings of the International Astronomical Union. 2006 ; Vol. 2, N.º S241. pp. 87-90.
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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.",
keywords = "Bulge, Population synthesis, Spectroscopy",
author = "B. Barbuy and A. Alves-Brito and M. Zoccali and D. Minniti and V. Hill and A. Lecureur and A. G{\'o}mez and S. Ortolani and A. Renzini and P. Coelho and L. Sodr{\'e}",
year = "2006",
month = "12",
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doi = "10.1017/S1743921307007491",
language = "English",
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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, vol. 2, n.º S241, pp. 87-90. https://doi.org/10.1017/S1743921307007491

Spectra of bulge stars with known abundance ratios for population synthesis. / Barbuy, B.; Alves-Brito, A.; Zoccali, M.; Minniti, D.; Hill, V.; Lecureur, A.; Gómez, A.; Ortolani, S.; Renzini, A.; Coelho, P.; Sodré, L.

En: Proceedings of the International Astronomical Union, Vol. 2, N.º S241, 01.12.2006, p. 87-90.

Resultado de la investigación: Article

TY - JOUR

T1 - Spectra of bulge stars with known abundance ratios for population synthesis

AU - Barbuy, B.

AU - Alves-Brito, A.

AU - Zoccali, M.

AU - Minniti, D.

AU - Hill, V.

AU - Lecureur, A.

AU - Gómez, A.

AU - Ortolani, S.

AU - Renzini, A.

AU - Coelho, P.

AU - Sodré, L.

PY - 2006/12/1

Y1 - 2006/12/1

N2 - 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.

AB - 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.

KW - Bulge

KW - Population synthesis

KW - Spectroscopy

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U2 - 10.1017/S1743921307007491

DO - 10.1017/S1743921307007491

M3 - Article

AN - SCOPUS:37149011956

VL - 2

SP - 87

EP - 90

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S241

ER -