Can T Tauri stars produce high-energy radiation?
- Autores
- del Valle, Maria Victoria; Romero, Gustavo Esteban
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- T Tauri stars are low mass, pre-main sequencestars. These objects are surrounded by an accretion disk and present strongmagnetic activity. T Tauri stars are copious X-rays emitters. The X-rays arelikely generated by powerful magnetic reconnection events.Strong shocks can be produced by massive reconnection in the stellar magnetosphere. These shocks or the reconnection of the field might accelerate particles up to relativistic energies, as observed in the Sun.We present a model for the high-energy radiation produced in themagnetosphere of T Tauri stars. We discuss whether this emission isdetectable with the existing gamma-ray telescopes.
Fil: del Valle, Maria Victoria. 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: 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
XIII Latin Aerican Regional IAU Meeting
Morelia
México
Universidad Nacional Autónoma de México - Materia
-
GAMMA RAYS: STARS
RADIATION MECHANISM: NON-THERMAL
STARS: PRE-MAIN SEQUENCE - 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:11336/150086
Ver los metadatos del registro completo
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Can T Tauri stars produce high-energy radiation?del Valle, Maria VictoriaRomero, Gustavo EstebanGAMMA RAYS: STARSRADIATION MECHANISM: NON-THERMALSTARS: PRE-MAIN SEQUENCEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1T Tauri stars are low mass, pre-main sequencestars. These objects are surrounded by an accretion disk and present strongmagnetic activity. T Tauri stars are copious X-rays emitters. The X-rays arelikely generated by powerful magnetic reconnection events.Strong shocks can be produced by massive reconnection in the stellar magnetosphere. These shocks or the reconnection of the field might accelerate particles up to relativistic energies, as observed in the Sun.We present a model for the high-energy radiation produced in themagnetosphere of T Tauri stars. We discuss whether this emission isdetectable with the existing gamma-ray telescopes.Fil: del Valle, Maria Victoria. 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: 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; ArgentinaXIII Latin Aerican Regional IAU MeetingMoreliaMéxicoUniversidad Nacional Autónoma de MéxicoUniversidad Nacional Autónoma de MéxicoHenney, Willian J.Torres Peimbert, Silvia2010info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/postscriptapplication/pdfhttp://hdl.handle.net/11336/150086Can T Tauri stars produce high-energy radiation?; XIII Latin Aerican Regional IAU Meeting; Morelia; México; 2010; 151-1521405-2059CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol40.htmlinfo:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..40/PDF/RMxAC..40_mdelvalle.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:28:45Zoai:ri.conicet.gov.ar:11336/150086instacron: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 10:28:46.151CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Can T Tauri stars produce high-energy radiation? |
title |
Can T Tauri stars produce high-energy radiation? |
spellingShingle |
Can T Tauri stars produce high-energy radiation? del Valle, Maria Victoria GAMMA RAYS: STARS RADIATION MECHANISM: NON-THERMAL STARS: PRE-MAIN SEQUENCE |
title_short |
Can T Tauri stars produce high-energy radiation? |
title_full |
Can T Tauri stars produce high-energy radiation? |
title_fullStr |
Can T Tauri stars produce high-energy radiation? |
title_full_unstemmed |
Can T Tauri stars produce high-energy radiation? |
title_sort |
Can T Tauri stars produce high-energy radiation? |
dc.creator.none.fl_str_mv |
del Valle, Maria Victoria Romero, Gustavo Esteban |
author |
del Valle, Maria Victoria |
author_facet |
del Valle, Maria Victoria Romero, Gustavo Esteban |
author_role |
author |
author2 |
Romero, Gustavo Esteban |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Henney, Willian J. Torres Peimbert, Silvia |
dc.subject.none.fl_str_mv |
GAMMA RAYS: STARS RADIATION MECHANISM: NON-THERMAL STARS: PRE-MAIN SEQUENCE |
topic |
GAMMA RAYS: STARS RADIATION MECHANISM: NON-THERMAL STARS: PRE-MAIN SEQUENCE |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
T Tauri stars are low mass, pre-main sequencestars. These objects are surrounded by an accretion disk and present strongmagnetic activity. T Tauri stars are copious X-rays emitters. The X-rays arelikely generated by powerful magnetic reconnection events.Strong shocks can be produced by massive reconnection in the stellar magnetosphere. These shocks or the reconnection of the field might accelerate particles up to relativistic energies, as observed in the Sun.We present a model for the high-energy radiation produced in themagnetosphere of T Tauri stars. We discuss whether this emission isdetectable with the existing gamma-ray telescopes. Fil: del Valle, Maria Victoria. 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: 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 XIII Latin Aerican Regional IAU Meeting Morelia México Universidad Nacional Autónoma de México |
description |
T Tauri stars are low mass, pre-main sequencestars. These objects are surrounded by an accretion disk and present strongmagnetic activity. T Tauri stars are copious X-rays emitters. The X-rays arelikely generated by powerful magnetic reconnection events.Strong shocks can be produced by massive reconnection in the stellar magnetosphere. These shocks or the reconnection of the field might accelerate particles up to relativistic energies, as observed in the Sun.We present a model for the high-energy radiation produced in themagnetosphere of T Tauri stars. We discuss whether this emission isdetectable with the existing gamma-ray telescopes. |
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/11336/150086 Can T Tauri stars produce high-energy radiation?; XIII Latin Aerican Regional IAU Meeting; Morelia; México; 2010; 151-152 1405-2059 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/150086 |
identifier_str_mv |
Can T Tauri stars produce high-energy radiation?; XIII Latin Aerican Regional IAU Meeting; Morelia; México; 2010; 151-152 1405-2059 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://www.astroscu.unam.mx/RMxAC/vol40.html info:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..40/PDF/RMxAC..40_mdelvalle.pdf |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/postscript application/pdf |
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Internacional |
dc.publisher.none.fl_str_mv |
Universidad Nacional Autónoma de México |
publisher.none.fl_str_mv |
Universidad Nacional Autónoma de México |
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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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13.070432 |