AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary

Autores
Gonzalez, Jorge Federico; Hubrig, S.; Nesvacil, N.; North, P.
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Using recent spectroscopic observations, we show that the triple system AO Vel with an eclipsing BpSi primary is in fact a remarkable quadruple system formed by two double-lined spectroscopic binaries with components close to the ZAMS. All available data have been reanalyzed to derive proper orbital parameters for both binary systems and to calculate absolute parameters of the eclipsing system. For the first time, direct determination of the radius and the mass have been obtained for a BpSi star. The study of the physical parameters of this unique system is especially important since it can be used as a test of evolutionary models for very young stars of intermediate mass.
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. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Hubrig, S.. European Southern Observatory Chile; Chile
Fil: Nesvacil, N.. European Southern Observatory Chile; Chile. Universidad de Viena; Austria
Fil: North, P.. École Polytechnique Fédérale de Lausanne; Suiza
Materia
STARS: BINARIES: SPECTROSCOPIC
STARS: CHEMICALLY PECULIAR
STARS: FUNDAMENTAL PARAMETERS
STARS: MAGNETIC FIELDS
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:11336/214858
Acceder
id CONICETDig_5188473189f5597b0e01ba9618e5c711
oai_identifier_str oai:ri.conicet.gov.ar:11336/214858
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primaryGonzalez, Jorge FedericoHubrig, S.Nesvacil, N.North, P.STARS: BINARIES: SPECTROSCOPICSTARS: CHEMICALLY PECULIARSTARS: FUNDAMENTAL PARAMETERSSTARS: MAGNETIC FIELDShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using recent spectroscopic observations, we show that the triple system AO Vel with an eclipsing BpSi primary is in fact a remarkable quadruple system formed by two double-lined spectroscopic binaries with components close to the ZAMS. All available data have been reanalyzed to derive proper orbital parameters for both binary systems and to calculate absolute parameters of the eclipsing system. For the first time, direct determination of the radius and the mass have been obtained for a BpSi star. The study of the physical parameters of this unique system is especially important since it can be used as a test of evolutionary models for very young stars of intermediate mass.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. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Hubrig, S.. European Southern Observatory Chile; ChileFil: Nesvacil, N.. European Southern Observatory Chile; Chile. Universidad de Viena; AustriaFil: North, P.. École Polytechnique Fédérale de Lausanne; SuizaEDP Sciences2006-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/214858Gonzalez, Jorge Federico; Hubrig, S.; Nesvacil, N.; North, P.; AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary; EDP Sciences; Astronomy and Astrophysics; 449; 1; 12-2006; 327-3340004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054103info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/13/aa4103-05/aa4103-05.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:01:14Zoai:ri.conicet.gov.ar:11336/214858instacron: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:34982025-10-22 11:01:14.636CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
title AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
spellingShingle AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
Gonzalez, Jorge Federico
STARS: BINARIES: SPECTROSCOPIC
STARS: CHEMICALLY PECULIAR
STARS: FUNDAMENTAL PARAMETERS
STARS: MAGNETIC FIELDS
title_short AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
title_full AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
title_fullStr AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
title_full_unstemmed AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
title_sort AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary
dc.creator.none.fl_str_mv Gonzalez, Jorge Federico
Hubrig, S.
Nesvacil, N.
North, P.
author Gonzalez, Jorge Federico
author_facet Gonzalez, Jorge Federico
Hubrig, S.
Nesvacil, N.
North, P.
author_role author
author2 Hubrig, S.
Nesvacil, N.
North, P.
author2_role author
author
author
dc.subject.none.fl_str_mv STARS: BINARIES: SPECTROSCOPIC
STARS: CHEMICALLY PECULIAR
STARS: FUNDAMENTAL PARAMETERS
STARS: MAGNETIC FIELDS
topic STARS: BINARIES: SPECTROSCOPIC
STARS: CHEMICALLY PECULIAR
STARS: FUNDAMENTAL PARAMETERS
STARS: MAGNETIC FIELDS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Using recent spectroscopic observations, we show that the triple system AO Vel with an eclipsing BpSi primary is in fact a remarkable quadruple system formed by two double-lined spectroscopic binaries with components close to the ZAMS. All available data have been reanalyzed to derive proper orbital parameters for both binary systems and to calculate absolute parameters of the eclipsing system. For the first time, direct determination of the radius and the mass have been obtained for a BpSi star. The study of the physical parameters of this unique system is especially important since it can be used as a test of evolutionary models for very young stars of intermediate mass.
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. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Hubrig, S.. European Southern Observatory Chile; Chile
Fil: Nesvacil, N.. European Southern Observatory Chile; Chile. Universidad de Viena; Austria
Fil: North, P.. École Polytechnique Fédérale de Lausanne; Suiza
description Using recent spectroscopic observations, we show that the triple system AO Vel with an eclipsing BpSi primary is in fact a remarkable quadruple system formed by two double-lined spectroscopic binaries with components close to the ZAMS. All available data have been reanalyzed to derive proper orbital parameters for both binary systems and to calculate absolute parameters of the eclipsing system. For the first time, direct determination of the radius and the mass have been obtained for a BpSi star. The study of the physical parameters of this unique system is especially important since it can be used as a test of evolutionary models for very young stars of intermediate mass.
publishDate 2006
dc.date.none.fl_str_mv 2006-12
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/11336/214858
Gonzalez, Jorge Federico; Hubrig, S.; Nesvacil, N.; North, P.; AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary; EDP Sciences; Astronomy and Astrophysics; 449; 1; 12-2006; 327-334
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/214858
identifier_str_mv Gonzalez, Jorge Federico; Hubrig, S.; Nesvacil, N.; North, P.; AO Velorum: A young quadruple system with a ZAMS eclipsing BpSi primary; EDP Sciences; Astronomy and Astrophysics; 449; 1; 12-2006; 327-334
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054103
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/13/aa4103-05/aa4103-05.html
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_ 1846781192308785152
score 12.982451

Publicaciones similares