Non-thermal radio emission from OB stars: an observer´s view

Autores
Benaglia, Paula
Año de publicación
2010
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments.
Fil: Benaglia, Paula. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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
High energy phenomena in Massive Stars
Jaén
España
Universidad de Jaén
Materia
MASSIVE STARS
RADIO CONTINUUM: NON THERMAL
COLLIDING WINDS
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:11336/231686
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Non-thermal radio emission from OB stars: an observer´s viewBenaglia, PaulaMASSIVE STARSRADIO CONTINUUM: NON THERMALCOLLIDING WINDShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments.Fil: Benaglia, Paula. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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; ArgentinaHigh energy phenomena in Massive StarsJaénEspañaUniversidad de JaénAstromical Society of the PacificMartí, JosepLuque Escamilla, Pedro L.Combi, Jorge Ariel2010info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/231686Non-thermal radio emission from OB stars: an observer´s view; High energy phenomena in Massive Stars; Jaén; España; 2009; 111-1229781583817247CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://aspbooks.org/custom/publications/paper/422-0111.htmlinfo:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2010ASPC..422..111B/abstractInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:02:47Zoai:ri.conicet.gov.ar:11336/231686instacron: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:34982025-10-22 11:02:47.671CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Non-thermal radio emission from OB stars: an observer´s view
title Non-thermal radio emission from OB stars: an observer´s view
spellingShingle Non-thermal radio emission from OB stars: an observer´s view
Benaglia, Paula
MASSIVE STARS
RADIO CONTINUUM: NON THERMAL
COLLIDING WINDS
title_short Non-thermal radio emission from OB stars: an observer´s view
title_full Non-thermal radio emission from OB stars: an observer´s view
title_fullStr Non-thermal radio emission from OB stars: an observer´s view
title_full_unstemmed Non-thermal radio emission from OB stars: an observer´s view
title_sort Non-thermal radio emission from OB stars: an observer´s view
dc.creator.none.fl_str_mv Benaglia, Paula
author Benaglia, Paula
author_facet Benaglia, Paula
author_role author
dc.contributor.none.fl_str_mv Martí, Josep
Luque Escamilla, Pedro L.
Combi, Jorge Ariel
dc.subject.none.fl_str_mv MASSIVE STARS
RADIO CONTINUUM: NON THERMAL
COLLIDING WINDS
topic MASSIVE STARS
RADIO CONTINUUM: NON THERMAL
COLLIDING WINDS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments.
Fil: Benaglia, Paula. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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
High energy phenomena in Massive Stars
Jaén
España
Universidad de Jaén
description Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments.
publishDate 2010
dc.date.none.fl_str_mv 2010
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Congreso
Journal
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/11336/231686
Non-thermal radio emission from OB stars: an observer´s view; High energy phenomena in Massive Stars; Jaén; España; 2009; 111-122
9781583817247
CONICET Digital
CONICET
url http://hdl.handle.net/11336/231686
identifier_str_mv Non-thermal radio emission from OB stars: an observer´s view; High energy phenomena in Massive Stars; Jaén; España; 2009; 111-122
9781583817247
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://aspbooks.org/custom/publications/paper/422-0111.html
info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2010ASPC..422..111B/abstract
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.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Astromical Society of the Pacific
publisher.none.fl_str_mv Astromical Society of the Pacific
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
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score 12.982451

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