HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary

Autores
Gonzalez, Jorge Federico; Saffe, Carlos; Castelli, F.; Hubrig, S.; Ilyin, I.; Schöller, M.; Carroll, T. A.; Leone, F.; Giarrusso, M.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, including the determination of physical parameters and photospheric chemical abundances.
Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Castelli, F.. Istituto Nazionale di Astrofisica. Osservatorio Astronomico di Trieste; Italia;
Fil: Hubrig, S.. Leibniz Institute for Astrophysics Potsdam; Alemania;
Fil: Ilyin, I.. Leibniz Institute for Astrophysics Potsdam, Alemania;
Fil: Schöller, M.. European Southern Observatory, Alemania;
Fil: Carroll, T. A.. Leibniz Institute for Astrophysics Potsdam, Alemania;
Fil: Leone, F.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia;
Fil: Giarrusso, M.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia; Osservatorio Astrofisico di Catania; Italia;
Materia
BINARYC
CHEMICALLY PECULIAR STARS
STARS ATMOSPHERES
STARS ABUNDANCES
MAGNETIC FIELD
INDIVIDUAL (HD161701)
SPECTROSCOPI
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/1640
Acceder
id CONICETDig_3d4c4aa1034e1eac881c2b1ae2adcd45
oai_identifier_str oai:ri.conicet.gov.ar:11336/1640
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondaryGonzalez, Jorge FedericoSaffe, CarlosCastelli, F.Hubrig, S.Ilyin, I.Schöller, M.Carroll, T. A.Leone, F.Giarrusso, M.BINARYCCHEMICALLY PECULIAR STARSSTARS ATMOSPHERESSTARS ABUNDANCESMAGNETIC FIELDINDIVIDUAL (HD161701)SPECTROSCOPIhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, including the determination of physical parameters and photospheric chemical abundances.Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;Fil: Castelli, F.. Istituto Nazionale di Astrofisica. Osservatorio Astronomico di Trieste; Italia;Fil: Hubrig, S.. Leibniz Institute for Astrophysics Potsdam; Alemania;Fil: Ilyin, I.. Leibniz Institute for Astrophysics Potsdam, Alemania;Fil: Schöller, M.. European Southern Observatory, Alemania;Fil: Carroll, T. A.. Leibniz Institute for Astrophysics Potsdam, Alemania;Fil: Leone, F.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia;Fil: Giarrusso, M.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia; Osservatorio Astrofisico di Catania; Italia;EDP Sciences2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/1640Gonzalez, Jorge Federico; Saffe, Carlos; Castelli, F.; Hubrig, S.; Ilyin, I.; et al.; HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary; EDP Sciences; Astronomy and Astrophysics; 561; 10-2013; 1-120004-6361enginfo:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/pdf/2014/01/aa22327-13.pdfinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201322327info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:38:16Zoai:ri.conicet.gov.ar:11336/1640instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:38:17.235CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
title HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
spellingShingle HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
Gonzalez, Jorge Federico
BINARYC
CHEMICALLY PECULIAR STARS
STARS ATMOSPHERES
STARS ABUNDANCES
MAGNETIC FIELD
INDIVIDUAL (HD161701)
SPECTROSCOPI
title_short HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
title_full HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
title_fullStr HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
title_full_unstemmed HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
title_sort HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
dc.creator.none.fl_str_mv Gonzalez, Jorge Federico
Saffe, Carlos
Castelli, F.
Hubrig, S.
Ilyin, I.
Schöller, M.
Carroll, T. A.
Leone, F.
Giarrusso, M.
author Gonzalez, Jorge Federico
author_facet Gonzalez, Jorge Federico
Saffe, Carlos
Castelli, F.
Hubrig, S.
Ilyin, I.
Schöller, M.
Carroll, T. A.
Leone, F.
Giarrusso, M.
author_role author
author2 Saffe, Carlos
Castelli, F.
Hubrig, S.
Ilyin, I.
Schöller, M.
Carroll, T. A.
Leone, F.
Giarrusso, M.
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv BINARYC
CHEMICALLY PECULIAR STARS
STARS ATMOSPHERES
STARS ABUNDANCES
MAGNETIC FIELD
INDIVIDUAL (HD161701)
SPECTROSCOPI
topic BINARYC
CHEMICALLY PECULIAR STARS
STARS ATMOSPHERES
STARS ABUNDANCES
MAGNETIC FIELD
INDIVIDUAL (HD161701)
SPECTROSCOPI
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, including the determination of physical parameters and photospheric chemical abundances.
Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - San Juan. Instituto de Ciencias Astronómicas de la Tierra y del Espacio; Argentina;
Fil: Castelli, F.. Istituto Nazionale di Astrofisica. Osservatorio Astronomico di Trieste; Italia;
Fil: Hubrig, S.. Leibniz Institute for Astrophysics Potsdam; Alemania;
Fil: Ilyin, I.. Leibniz Institute for Astrophysics Potsdam, Alemania;
Fil: Schöller, M.. European Southern Observatory, Alemania;
Fil: Carroll, T. A.. Leibniz Institute for Astrophysics Potsdam, Alemania;
Fil: Leone, F.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia;
Fil: Giarrusso, M.. Università di Catania. Dipartimento di Fisica e Astronomia. Sezione Astrofisica; Italia; Osservatorio Astrofisico di Catania; Italia;
description In recent years, HgMn stars have attracted attention after in several of them surface chemical spots of different elements were discovered, whose origin and possible connection with binarity and magnetic fields is not clear yet. Aims. We perform a complete study of the HgMn binary HD 161701, including the determination of physical parameters and photospheric chemical abundances.
publishDate 2013
dc.date.none.fl_str_mv 2013-10
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/11336/1640
Gonzalez, Jorge Federico; Saffe, Carlos; Castelli, F.; Hubrig, S.; Ilyin, I.; et al.; HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary; EDP Sciences; Astronomy and Astrophysics; 561; 10-2013; 1-12
0004-6361
url http://hdl.handle.net/11336/1640
identifier_str_mv Gonzalez, Jorge Federico; Saffe, Carlos; Castelli, F.; Hubrig, S.; Ilyin, I.; et al.; HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary; EDP Sciences; Astronomy and Astrophysics; 561; 10-2013; 1-12
0004-6361
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/pdf/2014/01/aa22327-13.pdf
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201322327
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1844613209220186112
score 13.070432

Publicaciones similares