Thermally Pulsing AGB Models of Intermediate Mass Stars
O. Straniero, M. Limongi, A. Chieffi, I. Dominguez, M. Busso, R. Gallino
Abstract
We present a set of models of AGB stars with initial mass larger than 5 Mo as obtained with the FRANEC code. It includes models of Z=0.02 and Z=0.001, with and without mass loss.
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