| Issue |
EAS Publications Series
Volume 63, 2013
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes
|
|
|---|---|---|
| Page(s) | 349 - 356 | |
| Section | Global Modelling of Stars | |
| DOI | https://doi.org/10.1051/eas/1363039 | |
| Published online | 19 December 2013 | |
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes
G. Alecian, Y. Lebreton, O. Richard and G. Vauclair (eds)
EAS Publications Series, 63 (2013) 349–356
G. Alecian, Y. Lebreton, O. Richard and G. Vauclair (eds)
EAS Publications Series, 63 (2013) 349–356
Stellar evolution including diffusion and matter flow induced by mass-loss
1 LUPM, Université Montpellier II, CNRS, cc072, Place E. Bataillon, 34095 Montpellier Cedex, France
2 Département de Physique, Université de Montréal, Montréal, Québec, H3C 3J7, Canada
It is clear that in order to explain many observed stellar phenomenae, atomic diffusion must be included in stellar models. Observed surface abundances allow us to constrain other transport pro- cesses which compete with atomic diffusion. We will focus on the effect of the flow of matter induced by mass-loss in stellar models.
© EAS, EDP Sciences, 2013