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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/214858
Ver los metadatos del registro completo
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 Técnicas2025-09-29T09:33:15Zoai: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:34982025-09-29 09:33:15.394CONICET 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_ |
1844613020386328576 |
score |
13.070432 |