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

We show that Montecarlo 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.

preprint2012arXivOpen access
Gustavo BruzualStephane CharlotRosa Gonzalez LopezliraSundar SrinivasanMartha L. BoyerDavid Riebel
astro-ph.CO
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Open access6 authors1 topic
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Gustavo BruzualStephane CharlotRosa Gonzalez LopezliraSundar SrinivasanMartha L. BoyerDavid Riebel

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