The s process in AGB stars as constrained by a large sample of barium stars

@article{Cseh2018TheSP,
  title={The s process in AGB stars as constrained by a large sample of barium stars},
  author={Borb'ala Cseh and Maria Lugaro and Valentina D’Orazi and Denise B. de Castro and Claudio Bastos Pereira and Amanda I. Karakas and L'aszl'o Moln'ar and Emese Plachy and R'obert Szab'o and Marco Pignatari and Sergio Cristallo},
  journal={Astronomy \& Astrophysics},
  year={2018}
}
Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produced by the slow neutron-capture process (s process). These stars belong to binary systems in which the primary star evolved through the asymptotic giant branch (AGB) phase. During this phase the primary star produced s-process elements and transferred them onto the secondary, which is now observed as a Ba star. Aims. We compare the largest homogeneous set of Ba giant star observations of the s… Expand

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