The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X

Autores
De Becker, M.; Rauw, G.; Pittard, J. M.; Blomme, R.; Romero, Gustavo Esteban; Sana, H.; Stevens, I. R.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, nonthermal emission processes such as inverse Compton (IC) scattering are expected to produce a high energy spectrum, in addition to the strong thermal emission from the shock-heated plasma. SIMBOL-X will be the ideal observatory to investigate the hard X-ray spectrum (above 10 keV) of these systems, i.e. where it is no longer dominated by the thermal emission. Such observations are strongly needed to constrain the models aimed at understanding the physics of particle acceleration in CWB. Such systems are important laboratories for investigating the underlying physics of particle acceleration at high Mach number shocks, and probe a different region of parameter space than studies of supernova remnants.
Fil: De Becker, M.. Universite de Liege; Bélgica
Fil: Rauw, G.. Universite de Liege; Bélgica
Fil: Pittard, J. M.. University of Leeds; Reino Unido
Fil: Blomme, R.. Royal Observatory of Belgium; Bélgica
Fil: Romero, Gustavo Esteban. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Sana, H.. European Southern Observatory; Chile
Fil: Stevens, I. R.. University of Birmingham; Reino Unido
Materia
Early Type Stars
Radiation Mechanisms
Non Thermal Mechanisms
X Ray Stars
Acceleration of Particles
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:11336/22954
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-XDe Becker, M.Rauw, G.Pittard, J. M.Blomme, R.Romero, Gustavo EstebanSana, H.Stevens, I. R.Early Type StarsRadiation MechanismsNon Thermal MechanismsX Ray StarsAcceleration of Particleshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, nonthermal emission processes such as inverse Compton (IC) scattering are expected to produce a high energy spectrum, in addition to the strong thermal emission from the shock-heated plasma. SIMBOL-X will be the ideal observatory to investigate the hard X-ray spectrum (above 10 keV) of these systems, i.e. where it is no longer dominated by the thermal emission. Such observations are strongly needed to constrain the models aimed at understanding the physics of particle acceleration in CWB. Such systems are important laboratories for investigating the underlying physics of particle acceleration at high Mach number shocks, and probe a different region of parameter space than studies of supernova remnants.Fil: De Becker, M.. Universite de Liege; BélgicaFil: Rauw, G.. Universite de Liege; BélgicaFil: Pittard, J. M.. University of Leeds; Reino UnidoFil: Blomme, R.. Royal Observatory of Belgium; BélgicaFil: Romero, Gustavo Esteban. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Sana, H.. European Southern Observatory; ChileFil: Stevens, I. R.. University of Birmingham; Reino UnidoSocietà Astronomica Italiana2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/22954De Becker, M.; Rauw, G.; Pittard, J. M.; Blomme, R.; Romero, Gustavo Esteban; et al.; The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X; Società Astronomica Italiana; Memorie della Società Astronomica Italiana; 79; 12-2008; 242-2431824-016XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MmSAI/79/PDF/242.pdfinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T10:05:19Zoai:ri.conicet.gov.ar:11336/22954instacron: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:34982025-09-03 10:05:19.612CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
title The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
spellingShingle The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
De Becker, M.
Early Type Stars
Radiation Mechanisms
Non Thermal Mechanisms
X Ray Stars
Acceleration of Particles
title_short The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
title_full The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
title_fullStr The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
title_full_unstemmed The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
title_sort The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X
dc.creator.none.fl_str_mv De Becker, M.
Rauw, G.
Pittard, J. M.
Blomme, R.
Romero, Gustavo Esteban
Sana, H.
Stevens, I. R.
author De Becker, M.
author_facet De Becker, M.
Rauw, G.
Pittard, J. M.
Blomme, R.
Romero, Gustavo Esteban
Sana, H.
Stevens, I. R.
author_role author
author2 Rauw, G.
Pittard, J. M.
Blomme, R.
Romero, Gustavo Esteban
Sana, H.
Stevens, I. R.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Early Type Stars
Radiation Mechanisms
Non Thermal Mechanisms
X Ray Stars
Acceleration of Particles
topic Early Type Stars
Radiation Mechanisms
Non Thermal Mechanisms
X Ray Stars
Acceleration of Particles
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, nonthermal emission processes such as inverse Compton (IC) scattering are expected to produce a high energy spectrum, in addition to the strong thermal emission from the shock-heated plasma. SIMBOL-X will be the ideal observatory to investigate the hard X-ray spectrum (above 10 keV) of these systems, i.e. where it is no longer dominated by the thermal emission. Such observations are strongly needed to constrain the models aimed at understanding the physics of particle acceleration in CWB. Such systems are important laboratories for investigating the underlying physics of particle acceleration at high Mach number shocks, and probe a different region of parameter space than studies of supernova remnants.
Fil: De Becker, M.. Universite de Liege; Bélgica
Fil: Rauw, G.. Universite de Liege; Bélgica
Fil: Pittard, J. M.. University of Leeds; Reino Unido
Fil: Blomme, R.. Royal Observatory of Belgium; Bélgica
Fil: Romero, Gustavo Esteban. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Sana, H.. European Southern Observatory; Chile
Fil: Stevens, I. R.. University of Birmingham; Reino Unido
description An increasing number of early-type (O and Wolf-Rayet) colliding wind binaries (CWBs) is known to accelerate particles up to relativistic energies. In this context, nonthermal emission processes such as inverse Compton (IC) scattering are expected to produce a high energy spectrum, in addition to the strong thermal emission from the shock-heated plasma. SIMBOL-X will be the ideal observatory to investigate the hard X-ray spectrum (above 10 keV) of these systems, i.e. where it is no longer dominated by the thermal emission. Such observations are strongly needed to constrain the models aimed at understanding the physics of particle acceleration in CWB. Such systems are important laboratories for investigating the underlying physics of particle acceleration at high Mach number shocks, and probe a different region of parameter space than studies of supernova remnants.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
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/11336/22954
De Becker, M.; Rauw, G.; Pittard, J. M.; Blomme, R.; Romero, Gustavo Esteban; et al.; The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X; Società Astronomica Italiana; Memorie della Società Astronomica Italiana; 79; 12-2008; 242-243
1824-016X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/22954
identifier_str_mv De Becker, M.; Rauw, G.; Pittard, J. M.; Blomme, R.; Romero, Gustavo Esteban; et al.; The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X; Società Astronomica Italiana; Memorie della Società Astronomica Italiana; 79; 12-2008; 242-243
1824-016X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MmSAI/79/PDF/242.pdf
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 Società Astronomica Italiana
publisher.none.fl_str_mv Società Astronomica Italiana
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_ 1842269905844436992
score 13.13397

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