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Thermally Pulsing AGB Models of Intermediate Mass Stars

O. Straniero·M. Limongi·A. Chieffi·I. Dominguez·M. Busso·R. Gallino
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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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O. Straniero, M. Limongi, A. Chieffi, I. Dominguez, M. Busso, R. Gallino. 1999-12-20. Thermally Pulsing AGB Models of Intermediate Mass Stars. https://arxiv.org/abs/astro-ph/9912426

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