High Energy Processes in Protostellar Jets

Autores
Rodríguez Kamenetzky, Adriana; Carrasco González, CAarlos; Araudo, Anabella Teresa; Torrelles, José María; Anglada, Guillem; Marti, Josep; Rodríguez, Luis Felipe; Valotto, Carlos
Año de publicación
2015
Idioma
español castellano
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
In the last years the presence of synchrotron emission has been proposed in a handful of protostellar jets. However, it is yet unclear how this "slow" jets could be able to accelerate particles up to relativistic velocities in order to emit detectable synchrotron emission. One of the most likely possibilities is that particles are accelerated in strong shocks of the jet against the dense envelopes surrounding the protostar. Particle acceleration has been studied in several astrophysical systems (AGN’s, microquasars, SN, massive binaries, etc.), nevertheless, in YSO is a fairly new phenomenon. Here, we present the analysis of high sensitivity continuum and linearly polarized images at several frequencies of one of the most characteristic non-thermal protostellar jets: The Triple Radio Source in Serpens.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/168048
Acceder
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spelling High Energy Processes in Protostellar JetsRodríguez Kamenetzky, AdrianaCarrasco González, CAarlosAraudo, Anabella TeresaTorrelles, José MaríaAnglada, GuillemMarti, JosepRodríguez, Luis FelipeValotto, CarlosCiencias Astronómicasprotostellar jetsThe Triple Radio Source in SerpensIn the last years the presence of synchrotron emission has been proposed in a handful of protostellar jets. However, it is yet unclear how this "slow" jets could be able to accelerate particles up to relativistic velocities in order to emit detectable synchrotron emission. One of the most likely possibilities is that particles are accelerated in strong shocks of the jet against the dense envelopes surrounding the protostar. Particle acceleration has been studied in several astrophysical systems (AGN’s, microquasars, SN, massive binaries, etc.), nevertheless, in YSO is a fairly new phenomenon. Here, we present the analysis of high sensitivity continuum and linearly polarized images at several frequencies of one of the most characteristic non-thermal protostellar jets: The Triple Radio Source in Serpens.Facultad de Ciencias Astronómicas y Geofísicas2015-10info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf105-110http://sedici.unlp.edu.ar/handle/10915/168048spainfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830info: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:UNLP2025-09-29T11:44:46Zoai:sedici.unlp.edu.ar:10915/168048Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:47.152SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv High Energy Processes in Protostellar Jets
title High Energy Processes in Protostellar Jets
spellingShingle High Energy Processes in Protostellar Jets
Rodríguez Kamenetzky, Adriana
Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
title_short High Energy Processes in Protostellar Jets
title_full High Energy Processes in Protostellar Jets
title_fullStr High Energy Processes in Protostellar Jets
title_full_unstemmed High Energy Processes in Protostellar Jets
title_sort High Energy Processes in Protostellar Jets
dc.creator.none.fl_str_mv Rodríguez Kamenetzky, Adriana
Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
author Rodríguez Kamenetzky, Adriana
author_facet Rodríguez Kamenetzky, Adriana
Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
author_role author
author2 Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
topic Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
dc.description.none.fl_txt_mv In the last years the presence of synchrotron emission has been proposed in a handful of protostellar jets. However, it is yet unclear how this "slow" jets could be able to accelerate particles up to relativistic velocities in order to emit detectable synchrotron emission. One of the most likely possibilities is that particles are accelerated in strong shocks of the jet against the dense envelopes surrounding the protostar. Particle acceleration has been studied in several astrophysical systems (AGN’s, microquasars, SN, massive binaries, etc.), nevertheless, in YSO is a fairly new phenomenon. Here, we present the analysis of high sensitivity continuum and linearly polarized images at several frequencies of one of the most characteristic non-thermal protostellar jets: The Triple Radio Source in Serpens.
Facultad de Ciencias Astronómicas y Geofísicas
description In the last years the presence of synchrotron emission has been proposed in a handful of protostellar jets. However, it is yet unclear how this "slow" jets could be able to accelerate particles up to relativistic velocities in order to emit detectable synchrotron emission. One of the most likely possibilities is that particles are accelerated in strong shocks of the jet against the dense envelopes surrounding the protostar. Particle acceleration has been studied in several astrophysical systems (AGN’s, microquasars, SN, massive binaries, etc.), nevertheless, in YSO is a fairly new phenomenon. Here, we present the analysis of high sensitivity continuum and linearly polarized images at several frequencies of one of the most characteristic non-thermal protostellar jets: The Triple Radio Source in Serpens.
publishDate 2015
dc.date.none.fl_str_mv 2015-10
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/168048
url http://sedici.unlp.edu.ar/handle/10915/168048
dc.language.none.fl_str_mv spa
language spa
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4
info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830
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
105-110
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
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