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Stellar Population Models

Published online by Cambridge University Press:  01 August 2006

Claudia Maraston
Claudia Maraston*
Affiliation:
University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK email: [email protected]
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Abstract

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I review the current status of stellar population modelling, with particular emphasis on the treatment of the Thermally-Pulsing Asymptotic Giant Branch stellar phase. I discuss how much the physical properties of galaxies that are derived applying these models to real data, depend on the adopted model.

Keywords

starsAGB and post-AGBgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 52 - 56
Copyright
Copyright © International Astronomical Union 2007

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