Non-thermal radiation from a runaway massive star
- Autores
- Romero, Gustavo Esteban; Benaglia, Paula; Peri, Cintia Soledad; Martí, Josep; Araudo, Anabella Teresa
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under the assumption that the reverse shock in the stellar wind might accelerate charged particles up to relativistic energies. Non-thermal radio emission of synchrotron origin has been detected, confirming the hypothesis. We have then modeled the system and we predict a spectral energy distribution that extends up to gamma-rays. Under some simplifying assumptions, we find that the intensity at high energies is too low to be detected by current instruments, but the future Cherenkov Telescope Array might detect the source.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Early-type stars
Cherenkov telescope array - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/99537
Ver los metadatos del registro completo
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Non-thermal radiation from a runaway massive starRomero, Gustavo EstebanBenaglia, PaulaPeri, Cintia SoledadMartí, JosepAraudo, Anabella TeresaCiencias AstronómicasEarly-type starsCherenkov telescope arrayWe present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under the assumption that the reverse shock in the stellar wind might accelerate charged particles up to relativistic energies. Non-thermal radio emission of synchrotron origin has been detected, confirming the hypothesis. We have then modeled the system and we predict a spectral energy distribution that extends up to gamma-rays. Under some simplifying assumptions, we find that the intensity at high energies is too low to be detected by current instruments, but the future Cherenkov Telescope Array might detect the source.Facultad de Ciencias Astronómicas y Geofísicas2011-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf420-424http://sedici.unlp.edu.ar/handle/10915/99537enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/5210info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1011.2773v1info:eu-repo/semantics/altIdentifier/issn/0037-9565info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1011.2773v1info:eu-repo/semantics/altIdentifier/arxiv/1011.2773v1info:eu-repo/semantics/altIdentifier/hdl/11336/5210info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:20:06Zoai:sedici.unlp.edu.ar:10915/99537Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:20:07.027SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Non-thermal radiation from a runaway massive star |
title |
Non-thermal radiation from a runaway massive star |
spellingShingle |
Non-thermal radiation from a runaway massive star Romero, Gustavo Esteban Ciencias Astronómicas Early-type stars Cherenkov telescope array |
title_short |
Non-thermal radiation from a runaway massive star |
title_full |
Non-thermal radiation from a runaway massive star |
title_fullStr |
Non-thermal radiation from a runaway massive star |
title_full_unstemmed |
Non-thermal radiation from a runaway massive star |
title_sort |
Non-thermal radiation from a runaway massive star |
dc.creator.none.fl_str_mv |
Romero, Gustavo Esteban Benaglia, Paula Peri, Cintia Soledad Martí, Josep Araudo, Anabella Teresa |
author |
Romero, Gustavo Esteban |
author_facet |
Romero, Gustavo Esteban Benaglia, Paula Peri, Cintia Soledad Martí, Josep Araudo, Anabella Teresa |
author_role |
author |
author2 |
Benaglia, Paula Peri, Cintia Soledad Martí, Josep Araudo, Anabella Teresa |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Early-type stars Cherenkov telescope array |
topic |
Ciencias Astronómicas Early-type stars Cherenkov telescope array |
dc.description.none.fl_txt_mv |
We present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under the assumption that the reverse shock in the stellar wind might accelerate charged particles up to relativistic energies. Non-thermal radio emission of synchrotron origin has been detected, confirming the hypothesis. We have then modeled the system and we predict a spectral energy distribution that extends up to gamma-rays. Under some simplifying assumptions, we find that the intensity at high energies is too low to be detected by current instruments, but the future Cherenkov Telescope Array might detect the source. Facultad de Ciencias Astronómicas y Geofísicas |
description |
We present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under the assumption that the reverse shock in the stellar wind might accelerate charged particles up to relativistic energies. Non-thermal radio emission of synchrotron origin has been detected, confirming the hypothesis. We have then modeled the system and we predict a spectral energy distribution that extends up to gamma-rays. Under some simplifying assumptions, we find that the intensity at high energies is too low to be detected by current instruments, but the future Cherenkov Telescope Array might detect the source. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-01 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/99537 |
url |
http://sedici.unlp.edu.ar/handle/10915/99537 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/5210 info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1011.2773v1 info:eu-repo/semantics/altIdentifier/issn/0037-9565 info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1011.2773v1 info:eu-repo/semantics/altIdentifier/arxiv/1011.2773v1 info:eu-repo/semantics/altIdentifier/hdl/11336/5210 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 420-424 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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