Nucleosynthesis in Intermediate-Mass Asymptotic Giant Branch Stars

Simple item page
dc.creatorLattanzio, John C.
dc.date1998-10-07
dc.date.accessioned2026-07-07T02:28:15Z
dc.date.available2026-07-07T02:28:15Z
dc.descriptionWe summarise the main properties of Asymptotic Giant Branch stars, including their structure, evolution and nucleosynthesis. The main physical mechanisms are outlined, as are the uncertainties. In keeping with the multi-disciplinary nature of this meeting, this paper is designed for those who are not experts in stellar structure.
dc.description7 pages, 3 figures, Invited Review presented at Nuclei in the Cosmos V, Volos, July 1998. For non-experts in stellar strucure! For related papers please see http://www.maths.monash.edu.au/~johnl/
dc.identifierhttps://arxiv.org/abs/astro-ph/9810094
dc.identifierhttp://arxiv.org/abs/astro-ph/9810094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13044
dc.subjectAstrophysics
dc.titleNucleosynthesis in Intermediate-Mass Asymptotic Giant Branch Stars
dc.typetext

Files

Collections

arXiv