Nucleosynthesis in intermediate mass AGB stars
| dc.creator | Lattanzio, John | |
| dc.creator | Charbonnel, Corinne | |
| dc.creator | Forestini, Manuel | |
| dc.date | 1999-12-15 | |
| dc.date.accessioned | 2026-07-07T02:34:59Z | |
| dc.date.available | 2026-07-07T02:34:59Z | |
| dc.description | We present a summary of the main sites for nucleosynthesis in intermediate mass Asymptotic Giant Branch (AGB) stars. We then discuss some detailed evolutionary models and how these have been used to create a synthetic evolution code which calculates the nucleosynthesis very rapidly, enabling us to investigate changes in some uncertain parameters in AGB evolution, such as mass-loss and dredge-up. We then present results for C, C/O, Mg and Al. We also discuss the changes due to the recent NACRE compilation of reaction rates. | |
| dc.description | 8 pages, including figures. Paper presented at Workshop on "The Changes in Abundances in Asymptotic Giant Branch Stars", Rome, Sept 16-18, 1999 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9912298 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9912298 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15462 | |
| dc.subject | Astrophysics | |
| dc.title | Nucleosynthesis in intermediate mass AGB stars | |
| dc.type | text |