Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation
- Autores
- De Becker, Michaël; Blomme, Ronny; Micela, Giusi; Pittard, Julian M.; Rauw, Gregor; Romero, Gustavo Esteban; Sana, Hugues; Stevens, Ian R.
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Several colliding-wind massive binaries are known to be non-thermal emitters in the radio domain. This constitutes strong evidence for the fact that an efficient particle acceleration process is at work in these objects. The acceleration mechanism is most probably the Diffusive Shock Acceleration (DSA) process in the presence of strong hydrodynamic shocks due to the colliding-winds. In order to investigate the physics of this particle acceleration, we initiated a multiwavelength campaign covering a large part of the electromagnetic spectrum. In this context, the detailed study of the hard X-ray emission from these sources in the SIMBOL-X bandpass constitutes a crucial element in order to probe this still poorly known topic of astrophysics. It should be noted that colliding-wind massive binaries should be considered as very valuable targets for the investigation of particle acceleration in a similar way as supernova remnants, but in a different region of the parameter space.
Fil: De Becker, Michaël. Université de Liège; Bélgica
Fil: Blomme, Ronny. Royal Observatory of Belgium; Bélgica
Fil: Micela, Giusi. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia
Fil: Pittard, Julian M.. University of Leeds; Reino Unido
Fil: Rauw, Gregor. Université de Liège; Bélgica
Fil: Romero, Gustavo Esteban. 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: Sana, Hugues. European Southern Obsevatory; Chile
Fil: Stevens, Ian R.. University Of Birmingham; Reino Unido
Simbol-X: focusing on the hard X-ray Universe
París, Francia
Francia
Universidade do Porto - Materia
-
Massive binaries
Colliding winds
SIMBOL-X - 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:11336/231473
Ver los metadatos del registro completo
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Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigationDe Becker, MichaëlBlomme, RonnyMicela, GiusiPittard, Julian M.Rauw, GregorRomero, Gustavo EstebanSana, HuguesStevens, Ian R.Massive binariesColliding windsSIMBOL-Xhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Several colliding-wind massive binaries are known to be non-thermal emitters in the radio domain. This constitutes strong evidence for the fact that an efficient particle acceleration process is at work in these objects. The acceleration mechanism is most probably the Diffusive Shock Acceleration (DSA) process in the presence of strong hydrodynamic shocks due to the colliding-winds. In order to investigate the physics of this particle acceleration, we initiated a multiwavelength campaign covering a large part of the electromagnetic spectrum. In this context, the detailed study of the hard X-ray emission from these sources in the SIMBOL-X bandpass constitutes a crucial element in order to probe this still poorly known topic of astrophysics. It should be noted that colliding-wind massive binaries should be considered as very valuable targets for the investigation of particle acceleration in a similar way as supernova remnants, but in a different region of the parameter space.Fil: De Becker, Michaël. Université de Liège; BélgicaFil: Blomme, Ronny. Royal Observatory of Belgium; BélgicaFil: Micela, Giusi. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; ItaliaFil: Pittard, Julian M.. University of Leeds; Reino UnidoFil: Rauw, Gregor. Université de Liège; BélgicaFil: Romero, Gustavo Esteban. 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: Sana, Hugues. European Southern Obsevatory; ChileFil: Stevens, Ian R.. University Of Birmingham; Reino UnidoSimbol-X: focusing on the hard X-ray UniverseParís, FranciaFranciaUniversidade do PortoAmerican Institute of Physics2009info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectConferenciaBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/231473Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation; Simbol-X: focusing on the hard X-ray Universe; París, Francia; Francia; 2008; 347-3509780735406629CONICET DigitalCONICETenghttps://sigarra.up.pt/fcup/en/pub_geral.pub_view?pi_pub_base_id=20012info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2009AIPC.1126..347D/abstractinfo:eu-repo/semantics/altIdentifier/doi/10.1063/1.3149450info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:43:04Zoai:ri.conicet.gov.ar:11336/231473instacron: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 09:43:04.486CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
title |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
spellingShingle |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation De Becker, Michaël Massive binaries Colliding winds SIMBOL-X |
title_short |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
title_full |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
title_fullStr |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
title_full_unstemmed |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
title_sort |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation |
dc.creator.none.fl_str_mv |
De Becker, Michaël Blomme, Ronny Micela, Giusi Pittard, Julian M. Rauw, Gregor Romero, Gustavo Esteban Sana, Hugues Stevens, Ian R. |
author |
De Becker, Michaël |
author_facet |
De Becker, Michaël Blomme, Ronny Micela, Giusi Pittard, Julian M. Rauw, Gregor Romero, Gustavo Esteban Sana, Hugues Stevens, Ian R. |
author_role |
author |
author2 |
Blomme, Ronny Micela, Giusi Pittard, Julian M. Rauw, Gregor Romero, Gustavo Esteban Sana, Hugues Stevens, Ian R. |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
Massive binaries Colliding winds SIMBOL-X |
topic |
Massive binaries Colliding winds SIMBOL-X |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Several colliding-wind massive binaries are known to be non-thermal emitters in the radio domain. This constitutes strong evidence for the fact that an efficient particle acceleration process is at work in these objects. The acceleration mechanism is most probably the Diffusive Shock Acceleration (DSA) process in the presence of strong hydrodynamic shocks due to the colliding-winds. In order to investigate the physics of this particle acceleration, we initiated a multiwavelength campaign covering a large part of the electromagnetic spectrum. In this context, the detailed study of the hard X-ray emission from these sources in the SIMBOL-X bandpass constitutes a crucial element in order to probe this still poorly known topic of astrophysics. It should be noted that colliding-wind massive binaries should be considered as very valuable targets for the investigation of particle acceleration in a similar way as supernova remnants, but in a different region of the parameter space. Fil: De Becker, Michaël. Université de Liège; Bélgica Fil: Blomme, Ronny. Royal Observatory of Belgium; Bélgica Fil: Micela, Giusi. Istituto Nazionale di Astrofísica. Osservatorio Astronómico di Palermo; Italia Fil: Pittard, Julian M.. University of Leeds; Reino Unido Fil: Rauw, Gregor. Université de Liège; Bélgica Fil: Romero, Gustavo Esteban. 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: Sana, Hugues. European Southern Obsevatory; Chile Fil: Stevens, Ian R.. University Of Birmingham; Reino Unido Simbol-X: focusing on the hard X-ray Universe París, Francia Francia Universidade do Porto |
description |
Several colliding-wind massive binaries are known to be non-thermal emitters in the radio domain. This constitutes strong evidence for the fact that an efficient particle acceleration process is at work in these objects. The acceleration mechanism is most probably the Diffusive Shock Acceleration (DSA) process in the presence of strong hydrodynamic shocks due to the colliding-winds. In order to investigate the physics of this particle acceleration, we initiated a multiwavelength campaign covering a large part of the electromagnetic spectrum. In this context, the detailed study of the hard X-ray emission from these sources in the SIMBOL-X bandpass constitutes a crucial element in order to probe this still poorly known topic of astrophysics. It should be noted that colliding-wind massive binaries should be considered as very valuable targets for the investigation of particle acceleration in a similar way as supernova remnants, but in a different region of the parameter space. |
publishDate |
2009 |
dc.date.none.fl_str_mv |
2009 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Conferencia Book http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
status_str |
publishedVersion |
format |
conferenceObject |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/231473 Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation; Simbol-X: focusing on the hard X-ray Universe; París, Francia; Francia; 2008; 347-350 9780735406629 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/231473 |
identifier_str_mv |
Non-thermal processes in colliding-wind massive binaries: the contribution of Simbol-X to a multiwavelength investigation; Simbol-X: focusing on the hard X-ray Universe; París, Francia; Francia; 2008; 347-350 9780735406629 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
https://sigarra.up.pt/fcup/en/pub_geral.pub_view?pi_pub_base_id=20012 info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2009AIPC.1126..347D/abstract info:eu-repo/semantics/altIdentifier/doi/10.1063/1.3149450 |
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 |
American Institute of Physics |
publisher.none.fl_str_mv |
American Institute of Physics |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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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 |
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13.070432 |