The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components

We present a study of the lithium abundances of a sample of evolved components of Chromospherically Active Binary Systems. We show that a significant part of them have lithium excesses, independently of their mass and evolutionary stage. Therefore, it can be concluded that Li abundance does not depe...

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Detalhes bibliográficos
Autores: Barrado y Navascués, D., Castro Rubio, Elisa De, Fernández Figueroa, María José, Cornide Castro-Piñeiro, Manuel, García López, R. J.
Formato: artículo
Fecha de publicación:1998
País:España
Recursos:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/59611
Acesso em linha:https://hdl.handle.net/20.500.14352/59611
Access Level:acceso abierto
Palavra-chave:52
RS-canum-venaticorum
Hyades cluster
CVN binaries
F-dwarfs
Stars
Abundances
Search
Scale
Astrofísica
Astronomía (Física)
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repository_id_str
spelling The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant componentsBarrado y Navascués, D.Castro Rubio, Elisa DeFernández Figueroa, María JoséCornide Castro-Piñeiro, ManuelGarcía López, R. J.52RS-canum-venaticorumHyades clusterCVN binariesF-dwarfsStarsAbundancesSearchScaleAstrofísicaAstronomía (Física)We present a study of the lithium abundances of a sample of evolved components of Chromospherically Active Binary Systems. We show that a significant part of them have lithium excesses, independently of their mass and evolutionary stage. Therefore, it can be concluded that Li abundance does not depend on age for giant components of CABS. These overabundances appear to be closely related to the stellar rotation, and we interpret them as a consequence of the transfer of angular momentum from the orbit to the rotation as the stars evolve: in and off the Main Sequence, in a similar way as it happens in the dwarf components of the same systems and in the Tidally Locked Binaries belonging to the Hyades and M67.EDP ScienciesUniversidad Complutense de Madrid19981998-09-2019981998-09-20journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/59611reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/596112026-06-02T12:44:21Z
dc.title.none.fl_str_mv The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
title The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
spellingShingle The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
Barrado y Navascués, D.
52
RS-canum-venaticorum
Hyades cluster
CVN binaries
F-dwarfs
Stars
Abundances
Search
Scale
Astrofísica
Astronomía (Física)
title_short The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
title_full The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
title_fullStr The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
title_full_unstemmed The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
title_sort The age-mass relation for chromospherically active binaries - III. Lithium depletion in giant components
dc.creator.none.fl_str_mv Barrado y Navascués, D.
Castro Rubio, Elisa De
Fernández Figueroa, María José
Cornide Castro-Piñeiro, Manuel
García López, R. J.
author Barrado y Navascués, D.
author_facet Barrado y Navascués, D.
Castro Rubio, Elisa De
Fernández Figueroa, María José
Cornide Castro-Piñeiro, Manuel
García López, R. J.
author_role author
author2 Castro Rubio, Elisa De
Fernández Figueroa, María José
Cornide Castro-Piñeiro, Manuel
García López, R. J.
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 52
RS-canum-venaticorum
Hyades cluster
CVN binaries
F-dwarfs
Stars
Abundances
Search
Scale
Astrofísica
Astronomía (Física)
topic 52
RS-canum-venaticorum
Hyades cluster
CVN binaries
F-dwarfs
Stars
Abundances
Search
Scale
Astrofísica
Astronomía (Física)
description We present a study of the lithium abundances of a sample of evolved components of Chromospherically Active Binary Systems. We show that a significant part of them have lithium excesses, independently of their mass and evolutionary stage. Therefore, it can be concluded that Li abundance does not depend on age for giant components of CABS. These overabundances appear to be closely related to the stellar rotation, and we interpret them as a consequence of the transfer of angular momentum from the orbit to the rotation as the stars evolve: in and off the Main Sequence, in a similar way as it happens in the dwarf components of the same systems and in the Tidally Locked Binaries belonging to the Hyades and M67.
publishDate 1998
dc.date.none.fl_str_mv 1998
1998-09-20
1998
1998-09-20
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/59611
url https://hdl.handle.net/20.500.14352/59611
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv EDP Sciencies
publisher.none.fl_str_mv EDP Sciencies
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869403479003365376
score 15.300719

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