Thermally Pulsing AGB Models of Intermediate Mass Stars
Astrophysics
2007-05-23 v1
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.
Cite
@article{arxiv.astro-ph/9912426,
title = {Thermally Pulsing AGB Models of Intermediate Mass Stars},
author = {O. Straniero and M. Limongi and A. Chieffi and I. Dominguez and M. Busso and R. Gallino},
journal= {arXiv preprint arXiv:astro-ph/9912426},
year = {2007}
}
Comments
9 pages, 9 figures (memsait.sty, epsf.sty) contribution to the workshop "The Changes in Abundances in Asymptotic Giant Branch Stars", held in Monte Porzio Catone (Italy), September 1999, to be published by Mem.Soc.Astron.It., eds. F. D'Antona and R. Gallino