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Beryllium, Lithium and Oxygen Abundances in F-type Stars

R. J. Garcia Lopez·M. C. Dominguez Herrera·M. R. Perez de Taoro·C. Casares·J. L. Rasilla·R. Rebolo·C. Allende Prieto
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Abstract

Beryllium and oxygen abundances have been derived in a sample of F-type field stars for which lithium abundances had been measured previously, with the aim of obtaining observational constraints to discriminate between the different mixing mechanisms proposed. Mixing associated with the transport of angular momentum in the stellar interior and internal gravity waves within the framework of rotating evolutionary models, appear to be promising ways to explain the observations.

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R. J. Garcia Lopez, M. C. Dominguez Herrera, M. R. Perez de Taoro, C. Casares, J. L. Rasilla, R. Rebolo, C. Allende Prieto. 1997-10-07. Beryllium, Lithium and Oxygen Abundances in F-type Stars. https://arxiv.org/abs/astro-ph/9710065

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