Thermally Pulsing AGB Models of Intermediate Mass Stars

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dc.creatorStraniero, O.
dc.creatorLimongi, M.
dc.creatorChieffi, A.
dc.creatorDominguez, I.
dc.creatorBusso, M.
dc.creatorGallino, R.
dc.date1999-12-20
dc.date.accessioned2026-07-07T02:35:07Z
dc.date.available2026-07-07T02:35:07Z
dc.descriptionWe 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.
dc.description9 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9912426
dc.identifierhttp://arxiv.org/abs/astro-ph/9912426
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15498
dc.subjectAstrophysics
dc.titleThermally Pulsing AGB Models of Intermediate Mass Stars
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