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The LF of TP-AGB stars in the LMC/SMC
Published online by Cambridge University Press: 17 July 2013
Abstract
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.
- 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