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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/27837
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:02:03Zoai: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:34982025-09-29 10:02:03.853CONICET 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 |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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