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Properties of young massive clusters obtained with different massive-star evolutionary models

Published online by Cambridge University Press:  27 October 2016

Aida Wofford  and
Stéphane Charlot
Aida Wofford
Affiliation:
UPMC-CNRS, UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris, France email: wofford@iap.fr, charlot@iap.fr
Stéphane Charlot
Affiliation:
UPMC-CNRS, UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris, France email: wofford@iap.fr, charlot@iap.fr
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Abstract

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We undertake a comprehensive comparative test of seven widely-used spectral synthesis models using multi-band HST photometry of a sample of eight YMCs in two galaxies. We provide a first quantitative estimate of the accuracies and uncertainties of new models, show the good progress of models in fitting high-quality observations, and highlight the need of further comprehensive comparative tests.

Keywords

(ISM:) Hii regionsgalaxies: star clusters: generalgalaxies: star formationultraviolet: galaxiesstars: early-type
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 186 - 187
Copyright
Copyright © International Astronomical Union 2016 

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