Bibcode
Garcia Lopez, R. J.; Dominguez Herrera, M. C.; Perez de Taoro, M. R.; Casares, C.; Rasilla, J. L.; Rebolo, R.; Allende Prieto, C.
Bibliographical reference
ASP Conf. Ser. 154, The Tenth Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, Edited by R. A. Donahue and J. A. Bookbinder, p.924
Advertised on:
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1998
Citations
0
Refereed citations
0
Description
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.