| Issue |
EAS Publications Series
Volume 63, 2013
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes
|
|
|---|---|---|
| Page(s) | 25 - 34 | |
| Section | Key Observations for Stellar Modelling | |
| DOI | https://doi.org/10.1051/eas/1363003 | |
| 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) 25–34
G. Alecian, Y. Lebreton, O. Richard and G. Vauclair (eds)
EAS Publications Series, 63 (2013) 25–34
CEMP-s and CEMP-s/r stars: last update
1 Department of Physics, University of Turin, Italy
2 INAF – Astrophysical Observatory Turin, Turin, Italy
3 B2FH Association-c/o Strada Osservatorio 20, 10023 Turin, Italy
4 INAF – Osservatorio Astronomico di Collurania, Teramo, Italy
5 KIT – Karlsruhe Institute of Technology, Karlsruhe, Germany
6 Department of Physics, University of Notre Dame, Notre Dame, IN, USA
We provide an updated discussion of the sample of CEMP-s and CEMP-s/r stars collected from the literature. Observations are compared with the theoretical nucleosynthesis models of asymptotic giant branch (AGB) stars presented by Bisterzo et al. (2010, 2011, 2012), in the light of the most recent spectroscopic results.
© EAS, EDP Sciences, 2013