Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-13T09:57:03.728Z Has data issue: false hasContentIssue false

Testing evolutionary synthesis models: Empirical feedback to model makers

Published online by Cambridge University Press:  13 April 2010

Roberto Cid Fernandes
Affiliation:
Departamento de Física-CFM, Universidade Federal de Santa Catarina, Florianópolis, Brasil
Rosa M. González Delgado
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Integrated spectra of star clusters are the best test beds for predictions of evolutionary synthesis models. We present spectral fits of star cluster using a variety of recent models. All models allow good spectral fits, but newer ones tend to be better. Ages estimated through spectral fits are not strongly model dependent, but metallicities can differ a lot from one model to another. For some clusters, multi-population fits suggest a combination of very old (1010 yr) and very young (< 108) populations, an artifact of the lack of old and blue stars in the models.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Bruzual, G. & Charlot, S. 2003, MNRAS, 344, 1000CrossRefGoogle Scholar
González Delgado, R. M., Cerviño, M., Martins, L. P., Leitherer, C., & Hauschildt, P. H. 2005, MNRAS, 357, 945CrossRefGoogle Scholar
Gomes, J. M. 2009, PhD thesis, Universidade Federal de Santa CatarinaGoogle Scholar
Leonardi, A. J. & Rose, J. A. 2003, ApJ, 126, 1811CrossRefGoogle Scholar
Koleva, M., Prugniel, Ph., Ocvirk, P., Le Borgne, D., & Soubiran, C. 2008, MNRAS, 385, 1998CrossRefGoogle Scholar
Martins, L. P., González Delgado, R. M., Leitherer, C., Cerviño, M., & Hauschildt, P. H. 2005, MNRAS, 358, 49CrossRefGoogle Scholar
Wolf, M. J., Drory, N., Gebhardt, K., & Hill, G. J. 2007, ApJ, 655, 179CrossRefGoogle Scholar