Radio Detection of Colliding Wind Binaries

Autores
Benaglia, Paula; Koribalski, Bärbel Silvia; Albacete Colombo, Juan Facundo
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Four massive, early-type stars, three of which are confirmed binaries, have been observed with theAustralia Telescope Compact Array at 1.4, 2.4, 4.8, and 8.6 GHz. The earliest star cataloged so far, HD 93129A,was also observed at 17.8 and 24.5 GHz. Here we present an analysis of the spectra as well as the structure of the stellar systems.All four spectra showclear evidence of non-thermal emission, indicative of a binary system with a colliding wind region. We discuss the magnetic field of the emitting region of HD 93129A and make predictions on the radiation at high energies. Archive X-ray observations towards the target sources are also investigated and interpreted in the light of the non-thermal emission detected.
Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Koribalski, Bärbel Silvia. Australia Telescope National Facility; Australia
Fil: Albacete Colombo, Juan Facundo. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
Early Type Stars
Cd-47 4551 (Estrella)
Mass Loss
Star Winds
Hd 93129a (Estrella)
Hd 124314 (Estrella)
Hd150136 (Estrella)
Outflows
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:11336/27837
Acceder
id CONICETDig_77430fb3be7b05b804d0101c7af00165
oai_identifier_str oai:ri.conicet.gov.ar:11336/27837
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Radio Detection of Colliding Wind BinariesBenaglia, PaulaKoribalski, Bärbel SilviaAlbacete Colombo, Juan FacundoEarly Type StarsCd-47 4551 (Estrella)Mass LossStar WindsHd 93129a (Estrella)Hd 124314 (Estrella)Hd150136 (Estrella)Outflowshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Four massive, early-type stars, three of which are confirmed binaries, have been observed with theAustralia Telescope Compact Array at 1.4, 2.4, 4.8, and 8.6 GHz. The earliest star cataloged so far, HD 93129A,was also observed at 17.8 and 24.5 GHz. Here we present an analysis of the spectra as well as the structure of the stellar systems.All four spectra showclear evidence of non-thermal emission, indicative of a binary system with a colliding wind region. We discuss the magnetic field of the emitting region of HD 93129A and make predictions on the radiation at high energies. Archive X-ray observations towards the target sources are also investigated and interpreted in the light of the non-thermal emission detected.Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Koribalski, Bärbel Silvia. Australia Telescope National Facility; AustraliaFil: Albacete Colombo, Juan Facundo. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaCambridge University Press2006-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/27837Benaglia, Paula; Koribalski, Bärbel Silvia; Albacete Colombo, Juan Facundo; Radio Detection of Colliding Wind Binaries ; Cambridge University Press; Publications Of The Astronomical Society Of Australia; 23; 1; 1-2006; 50-631323-3580CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1071/AS05039info:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/radio-detection-of-colliding-wind-binaries/262052168A12EC1525CD8139A42B0A48info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:58:07Zoai:ri.conicet.gov.ar:11336/27837instacron: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:34982025-10-15 14:58:08.233CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio Detection of Colliding Wind Binaries
title Radio Detection of Colliding Wind Binaries
spellingShingle Radio Detection of Colliding Wind Binaries
Benaglia, Paula
Early Type Stars
Cd-47 4551 (Estrella)
Mass Loss
Star Winds
Hd 93129a (Estrella)
Hd 124314 (Estrella)
Hd150136 (Estrella)
Outflows
title_short Radio Detection of Colliding Wind Binaries
title_full Radio Detection of Colliding Wind Binaries
title_fullStr Radio Detection of Colliding Wind Binaries
title_full_unstemmed Radio Detection of Colliding Wind Binaries
title_sort Radio Detection of Colliding Wind Binaries
dc.creator.none.fl_str_mv Benaglia, Paula
Koribalski, Bärbel Silvia
Albacete Colombo, Juan Facundo
author Benaglia, Paula
author_facet Benaglia, Paula
Koribalski, Bärbel Silvia
Albacete Colombo, Juan Facundo
author_role author
author2 Koribalski, Bärbel Silvia
Albacete Colombo, Juan Facundo
author2_role author
author
dc.subject.none.fl_str_mv Early Type Stars
Cd-47 4551 (Estrella)
Mass Loss
Star Winds
Hd 93129a (Estrella)
Hd 124314 (Estrella)
Hd150136 (Estrella)
Outflows
topic Early Type Stars
Cd-47 4551 (Estrella)
Mass Loss
Star Winds
Hd 93129a (Estrella)
Hd 124314 (Estrella)
Hd150136 (Estrella)
Outflows
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Four massive, early-type stars, three of which are confirmed binaries, have been observed with theAustralia Telescope Compact Array at 1.4, 2.4, 4.8, and 8.6 GHz. The earliest star cataloged so far, HD 93129A,was also observed at 17.8 and 24.5 GHz. Here we present an analysis of the spectra as well as the structure of the stellar systems.All four spectra showclear evidence of non-thermal emission, indicative of a binary system with a colliding wind region. We discuss the magnetic field of the emitting region of HD 93129A and make predictions on the radiation at high energies. Archive X-ray observations towards the target sources are also investigated and interpreted in the light of the non-thermal emission detected.
Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Koribalski, Bärbel Silvia. Australia Telescope National Facility; Australia
Fil: Albacete Colombo, Juan Facundo. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description Four massive, early-type stars, three of which are confirmed binaries, have been observed with theAustralia Telescope Compact Array at 1.4, 2.4, 4.8, and 8.6 GHz. The earliest star cataloged so far, HD 93129A,was also observed at 17.8 and 24.5 GHz. Here we present an analysis of the spectra as well as the structure of the stellar systems.All four spectra showclear evidence of non-thermal emission, indicative of a binary system with a colliding wind region. We discuss the magnetic field of the emitting region of HD 93129A and make predictions on the radiation at high energies. Archive X-ray observations towards the target sources are also investigated and interpreted in the light of the non-thermal emission detected.
publishDate 2006
dc.date.none.fl_str_mv 2006-01
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/11336/27837
Benaglia, Paula; Koribalski, Bärbel Silvia; Albacete Colombo, Juan Facundo; Radio Detection of Colliding Wind Binaries ; Cambridge University Press; Publications Of The Astronomical Society Of Australia; 23; 1; 1-2006; 50-63
1323-3580
CONICET Digital
CONICET
url http://hdl.handle.net/11336/27837
identifier_str_mv Benaglia, Paula; Koribalski, Bärbel Silvia; Albacete Colombo, Juan Facundo; Radio Detection of Colliding Wind Binaries ; Cambridge University Press; Publications Of The Astronomical Society Of Australia; 23; 1; 1-2006; 50-63
1323-3580
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1071/AS05039
info:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/radio-detection-of-colliding-wind-binaries/262052168A12EC1525CD8139A42B0A48
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
application/pdf
dc.publisher.none.fl_str_mv Cambridge University Press
publisher.none.fl_str_mv Cambridge University Press
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_ 1846083120977149952
score 13.22299

Publicaciones similares