KOLEVA, Mina; PRUGNIEL, Philippe; OCVIRK, Pierre; LE BORGNE, Damien; CHILINGARIAN, Igor; SOUBIRAN, C.

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KOLEVA, Mina
Софийски университет = Sofia University
Centre de Recherche Astrophysique de Lyon [CRAL]

PRUGNIEL, Philippe
Centre de Recherche Astrophysique de Lyon [CRAL]

OCVIRK, Pierre
Софийски университет = Sofia University

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Ce document a été publié dans

2007IAUS..241..183K - proceedings of IAU Symposium No. 241, 2007IAUS..241..183K - proceedings of IAU Symposium No. 241, "Stellar Populations as Building Blocks of Galaxies", 2006, la palma - Tenerife. 2007, vol. 241, p. 183-184

Cambridge University Press,

Résumé en anglais

We have compared simple stellar populations (SSPs) generated with different population synthesis tools: BC03, Vazdekis and Pegase.HR and different stellar libraries: ELODIE3.1, SteLib and MILES. We find that BC03/SteLib SSPs are biased toward solar metallicity, however Pegase.HR/ELODIE3.1 and Vazdekis/MILES are extremely consistent. The extensive coverage of the space of atmospheric parameters in the large stellar libraries allows precise synthesis for a large range of ages (0.1 .. 10 Gyr) and metallicities (-2 .. +0.4 dex) limited by the quality of the determination of stellar parameters (like temperature scale of the giants).< Réduire

Mots clés

galaxies: stellar content

galaxies: evolution

techniques: spectroscopic

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Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804