Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet
- Autores
- Sotomayor Checa, Pablo Omar; Romero, Gustavo Esteban
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In this work we propose a lepto-hadronic model for the non-thermal emission of the eastern jet of the galactic microquasar SS433. We obtain that the flux in TeV reported by the HAWK Collaboration can be explained by the decay of neutral pions produced in inelastic collisions proton-proton. Radio and X-ray emission is correctly fitted by synchrotron radiation of relativistic primary electrons.
En este trabajo proponemos un modelo lepto-hadrónico para la emisión no térmica del jet oriental del microcuásar galáctico SS433. Obtenemos que el flujo en TeV reportado por la Colaboración HAWK puede explicarse por el decaimiento de piones neutros producidos en colisiones inelásticas protón-protón. La emisión en radio y rayos X es correctamente modelada por radiación sincrotrón de electrones relativistas primarios.
Asociación Argentina de Astronomía - Materia
-
Ciencias Astronómicas
radiation mechanisms: non-thermal
stars: individial (SS433)
X-rays: binaries - 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:10915/176784
Ver los metadatos del registro completo
id |
SEDICI_818a219ef60f3065b3d052c5bc77619d |
---|---|
oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/176784 |
network_acronym_str |
SEDICI |
repository_id_str |
1329 |
network_name_str |
SEDICI (UNLP) |
spelling |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jetSotomayor Checa, Pablo OmarRomero, Gustavo EstebanCiencias Astronómicasradiation mechanisms: non-thermalstars: individial (SS433)X-rays: binariesIn this work we propose a lepto-hadronic model for the non-thermal emission of the eastern jet of the galactic microquasar SS433. We obtain that the flux in TeV reported by the HAWK Collaboration can be explained by the decay of neutral pions produced in inelastic collisions proton-proton. Radio and X-ray emission is correctly fitted by synchrotron radiation of relativistic primary electrons.En este trabajo proponemos un modelo lepto-hadrónico para la emisión no térmica del jet oriental del microcuásar galáctico SS433. Obtenemos que el flujo en TeV reportado por la Colaboración HAWK puede explicarse por el decaimiento de piones neutros producidos en colisiones inelásticas protón-protón. La emisión en radio y rayos X es correctamente modelada por radiación sincrotrón de electrones relativistas primarios.Asociación Argentina de Astronomía2021info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf271-273http://sedici.unlp.edu.ar/handle/10915/176784enginfo:eu-repo/semantics/altIdentifier/issn/1669-9521info: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:UNLP2025-09-29T11:47:44Zoai:sedici.unlp.edu.ar:10915/176784Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:47:44.36SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
title |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
spellingShingle |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet Sotomayor Checa, Pablo Omar Ciencias Astronómicas radiation mechanisms: non-thermal stars: individial (SS433) X-rays: binaries |
title_short |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
title_full |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
title_fullStr |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
title_full_unstemmed |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
title_sort |
Radiative model for the microquasar SS433: Non-thermal emission from the eastern jet |
dc.creator.none.fl_str_mv |
Sotomayor Checa, Pablo Omar Romero, Gustavo Esteban |
author |
Sotomayor Checa, Pablo Omar |
author_facet |
Sotomayor Checa, Pablo Omar Romero, Gustavo Esteban |
author_role |
author |
author2 |
Romero, Gustavo Esteban |
author2_role |
author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas radiation mechanisms: non-thermal stars: individial (SS433) X-rays: binaries |
topic |
Ciencias Astronómicas radiation mechanisms: non-thermal stars: individial (SS433) X-rays: binaries |
dc.description.none.fl_txt_mv |
In this work we propose a lepto-hadronic model for the non-thermal emission of the eastern jet of the galactic microquasar SS433. We obtain that the flux in TeV reported by the HAWK Collaboration can be explained by the decay of neutral pions produced in inelastic collisions proton-proton. Radio and X-ray emission is correctly fitted by synchrotron radiation of relativistic primary electrons. En este trabajo proponemos un modelo lepto-hadrónico para la emisión no térmica del jet oriental del microcuásar galáctico SS433. Obtenemos que el flujo en TeV reportado por la Colaboración HAWK puede explicarse por el decaimiento de piones neutros producidos en colisiones inelásticas protón-protón. La emisión en radio y rayos X es correctamente modelada por radiación sincrotrón de electrones relativistas primarios. Asociación Argentina de Astronomía |
description |
In this work we propose a lepto-hadronic model for the non-thermal emission of the eastern jet of the galactic microquasar SS433. We obtain that the flux in TeV reported by the HAWK Collaboration can be explained by the decay of neutral pions produced in inelastic collisions proton-proton. Radio and X-ray emission is correctly fitted by synchrotron radiation of relativistic primary electrons. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021 |
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/10915/176784 |
url |
http://sedici.unlp.edu.ar/handle/10915/176784 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1669-9521 |
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 271-273 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
reponame_str |
SEDICI (UNLP) |
collection |
SEDICI (UNLP) |
instname_str |
Universidad Nacional de La Plata |
instacron_str |
UNLP |
institution |
UNLP |
repository.name.fl_str_mv |
SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
_version_ |
1844616340465254400 |
score |
13.070432 |