Thermally Pulsing AGB Models of Intermediate Mass Stars
Straniero, O. · Limongi, M. · Chieffi, A. · Dominguez, I. · Busso, M. · Gallino, R.
Original · EN
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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