High-energy radiation from T-Tauri stars
- Autores
- Romero, Gustavo Esteban; del Valle, Maria Victoria; Martí, Josep; Luque Escamilla, Pedro L.
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are likely produced in the stellar magnetosphere by such events and charged particles accelerated up to relativistic energies. We present a simple model for the non-thermal radiation generated by high-energy particles in T Tauri stars. We discuss whether this emission is detectable at high energies with the available gamma-ray telescopes.
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: 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: Martí, Josep. Universidad de Jaén; España
Fil: Luque Escamilla, Pedro L.. Universidad de Jaén; España
25th Texas Symposium on Relativistic Astrophysics
Heidelberg
Alemania
Max-Planck-Institut für Kernphysik - Materia
-
T Tauri stars
non-thermal radiation
gamma-ray telescopes - 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:11336/225905
Ver los metadatos del registro completo
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High-energy radiation from T-Tauri starsRomero, Gustavo Estebandel Valle, Maria VictoriaMartí, JosepLuque Escamilla, Pedro L.T Tauri starsnon-thermal radiationgamma-ray telescopeshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are likely produced in the stellar magnetosphere by such events and charged particles accelerated up to relativistic energies. We present a simple model for the non-thermal radiation generated by high-energy particles in T Tauri stars. We discuss whether this emission is detectable at high energies with the available gamma-ray telescopes.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; ArgentinaFil: 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: Martí, Josep. Universidad de Jaén; EspañaFil: Luque Escamilla, Pedro L.. Universidad de Jaén; España25th Texas Symposium on Relativistic AstrophysicsHeidelbergAlemaniaMax-Planck-Institut für KernphysikSissa MedialabDingus, BrendaWagner, Stefan2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSimposioBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/225905High-energy radiation from T-Tauri stars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-6CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://pos.sissa.it/123/173info:eu-repo/semantics/altIdentifier/doi/10.22323/1.123.0173info:eu-repo/semantics/altIdentifier/url/https://www.mpi-hd.mpg.de/texas2010/Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:44:16Zoai:ri.conicet.gov.ar:11336/225905instacron: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 10:44:16.264CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
High-energy radiation from T-Tauri stars |
title |
High-energy radiation from T-Tauri stars |
spellingShingle |
High-energy radiation from T-Tauri stars Romero, Gustavo Esteban T Tauri stars non-thermal radiation gamma-ray telescopes |
title_short |
High-energy radiation from T-Tauri stars |
title_full |
High-energy radiation from T-Tauri stars |
title_fullStr |
High-energy radiation from T-Tauri stars |
title_full_unstemmed |
High-energy radiation from T-Tauri stars |
title_sort |
High-energy radiation from T-Tauri stars |
dc.creator.none.fl_str_mv |
Romero, Gustavo Esteban del Valle, Maria Victoria Martí, Josep Luque Escamilla, Pedro L. |
author |
Romero, Gustavo Esteban |
author_facet |
Romero, Gustavo Esteban del Valle, Maria Victoria Martí, Josep Luque Escamilla, Pedro L. |
author_role |
author |
author2 |
del Valle, Maria Victoria Martí, Josep Luque Escamilla, Pedro L. |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Dingus, Brenda Wagner, Stefan |
dc.subject.none.fl_str_mv |
T Tauri stars non-thermal radiation gamma-ray telescopes |
topic |
T Tauri stars non-thermal radiation gamma-ray telescopes |
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 young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are likely produced in the stellar magnetosphere by such events and charged particles accelerated up to relativistic energies. We present a simple model for the non-thermal radiation generated by high-energy particles in T Tauri stars. We discuss whether this emission is detectable at high energies with the available gamma-ray telescopes. 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: 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: Martí, Josep. Universidad de Jaén; España Fil: Luque Escamilla, Pedro L.. Universidad de Jaén; España 25th Texas Symposium on Relativistic Astrophysics Heidelberg Alemania Max-Planck-Institut für Kernphysik |
description |
T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are likely produced in the stellar magnetosphere by such events and charged particles accelerated up to relativistic energies. We present a simple model for the non-thermal radiation generated by high-energy particles in T Tauri stars. We discuss whether this emission is detectable at high energies with the available gamma-ray telescopes. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Simposio 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/11336/225905 High-energy radiation from T-Tauri stars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-6 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/225905 |
identifier_str_mv |
High-energy radiation from T-Tauri stars; 25th Texas Symposium on Relativistic Astrophysics; Heidelberg; Alemania; 2010; 1-6 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://pos.sissa.it/123/173 info:eu-repo/semantics/altIdentifier/doi/10.22323/1.123.0173 info:eu-repo/semantics/altIdentifier/url/https://www.mpi-hd.mpg.de/texas2010/ |
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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 |
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Sissa Medialab |
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Sissa Medialab |
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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 |
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