Progresses in AGB Modelling

Author(s)
Sergio Cristallo, Oscar Straniero, Roberto Gallino, Michael Lederer, L. Piersanti, I. Domínguez
Abstract

The full understanding of final stellar evolution phases is a fundamental request to properly investigate the Universe at any temporal and spatial scale. While the theoretical scenarios of H- and He-burning have been deeply investigated in the last 30 years, the modelling of stellar evolution beyond the core-helium burning phase and the related nucleosynthesis still present problems related to the physics and to the numerical methods. Low mass AGB Stars (1

Organisation(s)
Department of Astrophysics
External organisation(s)
Osservatorio Astronomico di Collurania-Teramo, Universidad de Granada, University of Turin, Osservatorio Astronomico di Collurania Vincenzo Cerulli
Pages
3-10
No. of pages
8
DOI
https://doi.org/10.1063/1.2916987
Publication date
2008
Austrian Fields of Science 2012
1030 Physics, Astronomy
Portal url
https://ucrisportal.univie.ac.at/en/publications/55f55776-3904-42c8-a037-72d4756bcb24