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Stellar Population Models

Published online by Cambridge University Press:  17 July 2013

Claudia Maraston
Claudia Maraston*
Affiliation:
Institute of Cosmology and Gravitation, University of Portsmouth, Burnaby Road, PO1 3FX, Portsmouth, United Kingdom email: claudia.maraston@port.ac.uk
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Abstract

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Modelling stellar populations in galaxies is a key approach to gain knowledge on the still elusive process of galaxy formation as a function of cosmic time. In this review, after a summary of the state-of-art, I discuss three aspects of the modelling, that are particularly relevant to massive galaxies, the focus of this symposium, at low and high-redshift. These are the treatment of the Thermally-Pulsating Asymptotic Giant Branch phase, evidences of an unusual Initial Mass Function, and the effect of modern stellar libraries on the model spectral energy distribution.

Keywords

galaxies: formationgalaxies: evolutiongalaxies: high-redshiftgalaxies: spiralgalaxies: initial mass functionstars: AGB and post-AGBstars: atmospheresstars: carbon
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 272 - 281
Copyright
Copyright © International Astronomical Union 2013 

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