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The LF of TP-AGB stars in the LMC/SMC

Published online by Cambridge University Press:  17 July 2013

Gustavo Bruzual ,
Stéphane Charlot ,
Rosa González Lópezlira ,
Sundar Srinivasan ,
Martha L. Boyer  and
David Riebel
Gustavo Bruzual
Affiliation:
Centro de Radioastronomía y Astrofísica, UNAM, Campus Morelia, México email: [email protected], [email protected]
Stéphane Charlot
Affiliation:
UPMC, UMR7095, Institut d'Astrophysique de Paris, F-75014, Paris, France CNRS, UMR7095, Institut d'Astrophysique de Paris, F-75014, Paris, France email: [email protected]
Rosa González Lópezlira
Affiliation:
Centro de Radioastronomía y Astrofísica, UNAM, Campus Morelia, México email: [email protected], [email protected]
Sundar Srinivasan
Affiliation:
Academia Sinica, Institute of Astronomy and Astrophysics, PO Box 23-141, Taipei 10617, Taiwan, R. O. C., email: [email protected]
Martha L. Boyer
Affiliation:
STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA, email: [email protected]
David Riebel
Affiliation:
Department of Physics, United States Naval Academy, 572C Holloway Road, Annapolis, MD 21402, USA, email: [email protected]
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Abstract

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We show that Monte Carlo simulations of the TP-AGB stellar population in the LMC and SMC galaxies using the CB* models produce LF and color distributions that are in closer agreement with observations than those obtained with the BC03 and CB07 models. This is a progress report of work that will be published elsewhere.

Keywords

stars: evolutionstars: AGB and post-AGBgalaxies: stellar contentgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 282 - 285
Copyright
Copyright © International Astronomical Union 2013 

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