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CEMP-s and CEMP-s/r stars: last update

Published online by Cambridge University Press:  19 December 2013

S. Bisterzo ,
R. Gallino ,
O. Straniero ,
S. Cristallo ,
F. Käppeler  and
M. Wiescher
S. Bisterzo
Affiliation:
Department of Physics, University of Turin, Italy INAF – Astrophysical Observatory Turin, Turin, Italy
R. Gallino
Affiliation:
Department of Physics, University of Turin, Italy B2FH Association-c/o Strada Osservatorio 20, 10023 Turin, Italy
O. Straniero
Affiliation:
INAF – Osservatorio Astronomico di Collurania, Teramo, Italy
S. Cristallo
Affiliation:
B2FH Association-c/o Strada Osservatorio 20, 10023 Turin, Italy
F. Käppeler
Affiliation:
KIT – Karlsruhe Institute of Technology, Karlsruhe, Germany
M. Wiescher
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA
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Abstract

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.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 63: New Advances in Stellar Physics: From Microscopic to Macroscopic Processes , 2013 , pp. 25 - 34
Copyright
© EAS, EDP Sciences, 2013

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