Beryllium, Lithium and Oxygen Abundances in F-type Stars

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dc.creatorLopez, R. J. Garcia
dc.creatorHerrera, M. C. Dominguez
dc.creatorde Taoro, M. R. Perez
dc.creatorCasares, C.
dc.creatorRasilla, J. L.
dc.creatorRebolo, R.
dc.creatorPrieto, C. Allende
dc.date1997-10-07
dc.date.accessioned2026-07-07T02:24:26Z
dc.date.available2026-07-07T02:24:26Z
dc.descriptionBeryllium 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.
dc.descriptionLatex file (8 pages), uses html.sty, epsf.sty and cs10.sty (included); 3 EPS figures. To appear in the Proceedings of the 10th Cambridge Workshop Cool Stars, Stellar Systems and the Sun (Cambridge, MA USA, July 1997)
dc.identifierhttps://arxiv.org/abs/astro-ph/9710065
dc.identifierhttp://arxiv.org/abs/astro-ph/9710065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11618
dc.subjectAstrophysics
dc.titleBeryllium, Lithium and Oxygen Abundances in F-type Stars
dc.typetext

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