Elemental abundance study of the CP star HD 206653

Autores
Albacete-Colombo, J.F.; López-García, Z.; Levato, H.; Malaroda, S.M.; Grosso, M.
Año de publicación
2002
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors.
Fuente
Astron. Astrophys. 2002;392(2):613-617
Materia
Stars: abundances
Stars: chemically peculiar
Stars: individual: HD 206653
Airborne telescopes
Cerium
Europium
Mathematical models
Rare earths
Silicon
Solar system
Iron peak elements
Light elements
Stars
Astrophysics
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/2.5/ar
Repositorio
Biblioteca Digital (UBA-FCEN)
Institución
Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
OAI Identificador
paperaa:paper_00046361_v392_n2_p613_AlbaceteColombo
Acceder
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oai_identifier_str paperaa:paper_00046361_v392_n2_p613_AlbaceteColombo
network_acronym_str BDUBAFCEN
repository_id_str 1896
network_name_str Biblioteca Digital (UBA-FCEN)
spelling Elemental abundance study of the CP star HD 206653Albacete-Colombo, J.F.López-García, Z.Levato, H.Malaroda, S.M.Grosso, M.Stars: abundancesStars: chemically peculiarStars: individual: HD 206653Airborne telescopesCeriumEuropiumMathematical modelsRare earthsSiliconSolar systemIron peak elementsLight elementsStarsAstrophysicsAn analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors.2002info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/20.500.12110/paper_00046361_v392_n2_p613_AlbaceteColomboAstron. Astrophys. 2002;392(2):613-617reponame:Biblioteca Digital (UBA-FCEN)instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesinstacron:UBA-FCENenginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/2.5/ar2025-09-29T13:43:09Zpaperaa:paper_00046361_v392_n2_p613_AlbaceteColomboInstitucionalhttps://digital.bl.fcen.uba.ar/Universidad públicaNo correspondehttps://digital.bl.fcen.uba.ar/cgi-bin/oaiserver.cgiana@bl.fcen.uba.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:18962025-09-29 13:43:10.624Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesfalse
dc.title.none.fl_str_mv Elemental abundance study of the CP star HD 206653
title Elemental abundance study of the CP star HD 206653
spellingShingle Elemental abundance study of the CP star HD 206653
Albacete-Colombo, J.F.
Stars: abundances
Stars: chemically peculiar
Stars: individual: HD 206653
Airborne telescopes
Cerium
Europium
Mathematical models
Rare earths
Silicon
Solar system
Iron peak elements
Light elements
Stars
Astrophysics
title_short Elemental abundance study of the CP star HD 206653
title_full Elemental abundance study of the CP star HD 206653
title_fullStr Elemental abundance study of the CP star HD 206653
title_full_unstemmed Elemental abundance study of the CP star HD 206653
title_sort Elemental abundance study of the CP star HD 206653
dc.creator.none.fl_str_mv Albacete-Colombo, J.F.
López-García, Z.
Levato, H.
Malaroda, S.M.
Grosso, M.
author Albacete-Colombo, J.F.
author_facet Albacete-Colombo, J.F.
López-García, Z.
Levato, H.
Malaroda, S.M.
Grosso, M.
author_role author
author2 López-García, Z.
Levato, H.
Malaroda, S.M.
Grosso, M.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Stars: abundances
Stars: chemically peculiar
Stars: individual: HD 206653
Airborne telescopes
Cerium
Europium
Mathematical models
Rare earths
Silicon
Solar system
Iron peak elements
Light elements
Stars
Astrophysics
topic Stars: abundances
Stars: chemically peculiar
Stars: individual: HD 206653
Airborne telescopes
Cerium
Europium
Mathematical models
Rare earths
Silicon
Solar system
Iron peak elements
Light elements
Stars
Astrophysics
dc.description.none.fl_txt_mv An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors.
description An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors.
publishDate 2002
dc.date.none.fl_str_mv 2002
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/20.500.12110/paper_00046361_v392_n2_p613_AlbaceteColombo
url http://hdl.handle.net/20.500.12110/paper_00046361_v392_n2_p613_AlbaceteColombo
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/2.5/ar
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv Astron. Astrophys. 2002;392(2):613-617
reponame:Biblioteca Digital (UBA-FCEN)
instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron:UBA-FCEN
reponame_str Biblioteca Digital (UBA-FCEN)
collection Biblioteca Digital (UBA-FCEN)
instname_str Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron_str UBA-FCEN
institution UBA-FCEN
repository.name.fl_str_mv Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
repository.mail.fl_str_mv ana@bl.fcen.uba.ar
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score 13.070432

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