Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens

Autores
Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Torrelles, Jose M.; Anglada, Guillem; Marti, Josep; Luis Felipe Rodriguez; Valotto, Carlos Alberto
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
While most protostellar jets present free-free emission at radio wavelengths, synchrotron emission has also been proposed to be present in a handful of these objects. The presence of nonthermal emission has been inferred by negative spectral indices at centimeter wavelengths. In one case (the HH 80-81 jet arising from a massive protostar), its synchrotron nature was confirmed by the detection of linearly polarized radio emission. One of the main consequences of these results is that synchrotron emission implies the presence of relativistic particles among the nonrelativistic material of these jets. Therefore, an acceleration mechanism should be taking place. The most probable scenario is that particles are accelerated when the jets strongly impact against the dense envelope surrounding the protostar. Here we present an analysis of radio observations obtained with the Very Large Array of the triple radio source in the Serpens star-forming region. This object is known to be a radio jet arising from an intermediate-mass protostar. It is also one of the first protostellar jets where the presence of nonthermal emission was proposed. We analyze the dynamics of the jet and the nature of the emission and discuss these issues in the context of the physical parameters of the jet and the particle acceleration phenomenon.
Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Carrasco Gonzalez, Carlos Eugenio. Universidad Nacional Autónoma de México; México
Fil: Araudo, Anabella Teresa. University of Oxford. Department of Physics; Reino Unido. 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: Torrelles, Jose M.. Universidad de Barcelona; España
Fil: Anglada, Guillem. Instituto de Astrofisica Andalucia; España
Fil: Marti, Josep. Universidad de Jaén; España
Fil: Luis Felipe Rodriguez. Universidad Nacional Autónoma de México; México
Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Materia
ACCELERATION OF PARTICLES
ISM: JETS AND OUTFLOWS
ISM: KINEMATICS AND DYNAMICS
ISM: MAGNETIC FIELDS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/183020
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpensRodríguez Kamenetzky, Adriana RaquelCarrasco Gonzalez, Carlos EugenioAraudo, Anabella TeresaTorrelles, Jose M.Anglada, GuillemMarti, JosepLuis Felipe RodriguezValotto, Carlos AlbertoACCELERATION OF PARTICLESISM: JETS AND OUTFLOWSISM: KINEMATICS AND DYNAMICSISM: MAGNETIC FIELDShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1While most protostellar jets present free-free emission at radio wavelengths, synchrotron emission has also been proposed to be present in a handful of these objects. The presence of nonthermal emission has been inferred by negative spectral indices at centimeter wavelengths. In one case (the HH 80-81 jet arising from a massive protostar), its synchrotron nature was confirmed by the detection of linearly polarized radio emission. One of the main consequences of these results is that synchrotron emission implies the presence of relativistic particles among the nonrelativistic material of these jets. Therefore, an acceleration mechanism should be taking place. The most probable scenario is that particles are accelerated when the jets strongly impact against the dense envelope surrounding the protostar. Here we present an analysis of radio observations obtained with the Very Large Array of the triple radio source in the Serpens star-forming region. This object is known to be a radio jet arising from an intermediate-mass protostar. It is also one of the first protostellar jets where the presence of nonthermal emission was proposed. We analyze the dynamics of the jet and the nature of the emission and discuss these issues in the context of the physical parameters of the jet and the particle acceleration phenomenon.Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Carrasco Gonzalez, Carlos Eugenio. Universidad Nacional Autónoma de México; MéxicoFil: Araudo, Anabella Teresa. University of Oxford. Department of Physics; Reino Unido. 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: Torrelles, Jose M.. Universidad de Barcelona; EspañaFil: Anglada, Guillem. Instituto de Astrofisica Andalucia; EspañaFil: Marti, Josep. Universidad de Jaén; EspañaFil: Luis Felipe Rodriguez. Universidad Nacional Autónoma de México; MéxicoFil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaIOP Publishing2016-02-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/183020Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Torrelles, Jose M.; Anglada, Guillem; et al.; Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens; IOP Publishing; Astrophysical Journal; 818; 1; 4-2-2016; 1-250004-637X1538-4357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/0004-637X/818/1/27info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/818/1/27info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:00:55Zoai:ri.conicet.gov.ar:11336/183020instacron: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 10:00:55.777CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
title Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
spellingShingle Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
Rodríguez Kamenetzky, Adriana Raquel
ACCELERATION OF PARTICLES
ISM: JETS AND OUTFLOWS
ISM: KINEMATICS AND DYNAMICS
ISM: MAGNETIC FIELDS
title_short Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
title_full Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
title_fullStr Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
title_full_unstemmed Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
title_sort Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens
dc.creator.none.fl_str_mv Rodríguez Kamenetzky, Adriana Raquel
Carrasco Gonzalez, Carlos Eugenio
Araudo, Anabella Teresa
Torrelles, Jose M.
Anglada, Guillem
Marti, Josep
Luis Felipe Rodriguez
Valotto, Carlos Alberto
author Rodríguez Kamenetzky, Adriana Raquel
author_facet Rodríguez Kamenetzky, Adriana Raquel
Carrasco Gonzalez, Carlos Eugenio
Araudo, Anabella Teresa
Torrelles, Jose M.
Anglada, Guillem
Marti, Josep
Luis Felipe Rodriguez
Valotto, Carlos Alberto
author_role author
author2 Carrasco Gonzalez, Carlos Eugenio
Araudo, Anabella Teresa
Torrelles, Jose M.
Anglada, Guillem
Marti, Josep
Luis Felipe Rodriguez
Valotto, Carlos Alberto
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ACCELERATION OF PARTICLES
ISM: JETS AND OUTFLOWS
ISM: KINEMATICS AND DYNAMICS
ISM: MAGNETIC FIELDS
topic ACCELERATION OF PARTICLES
ISM: JETS AND OUTFLOWS
ISM: KINEMATICS AND DYNAMICS
ISM: MAGNETIC FIELDS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv While most protostellar jets present free-free emission at radio wavelengths, synchrotron emission has also been proposed to be present in a handful of these objects. The presence of nonthermal emission has been inferred by negative spectral indices at centimeter wavelengths. In one case (the HH 80-81 jet arising from a massive protostar), its synchrotron nature was confirmed by the detection of linearly polarized radio emission. One of the main consequences of these results is that synchrotron emission implies the presence of relativistic particles among the nonrelativistic material of these jets. Therefore, an acceleration mechanism should be taking place. The most probable scenario is that particles are accelerated when the jets strongly impact against the dense envelope surrounding the protostar. Here we present an analysis of radio observations obtained with the Very Large Array of the triple radio source in the Serpens star-forming region. This object is known to be a radio jet arising from an intermediate-mass protostar. It is also one of the first protostellar jets where the presence of nonthermal emission was proposed. We analyze the dynamics of the jet and the nature of the emission and discuss these issues in the context of the physical parameters of the jet and the particle acceleration phenomenon.
Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Carrasco Gonzalez, Carlos Eugenio. Universidad Nacional Autónoma de México; México
Fil: Araudo, Anabella Teresa. University of Oxford. Department of Physics; Reino Unido. 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: Torrelles, Jose M.. Universidad de Barcelona; España
Fil: Anglada, Guillem. Instituto de Astrofisica Andalucia; España
Fil: Marti, Josep. Universidad de Jaén; España
Fil: Luis Felipe Rodriguez. Universidad Nacional Autónoma de México; México
Fil: Valotto, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
description While most protostellar jets present free-free emission at radio wavelengths, synchrotron emission has also been proposed to be present in a handful of these objects. The presence of nonthermal emission has been inferred by negative spectral indices at centimeter wavelengths. In one case (the HH 80-81 jet arising from a massive protostar), its synchrotron nature was confirmed by the detection of linearly polarized radio emission. One of the main consequences of these results is that synchrotron emission implies the presence of relativistic particles among the nonrelativistic material of these jets. Therefore, an acceleration mechanism should be taking place. The most probable scenario is that particles are accelerated when the jets strongly impact against the dense envelope surrounding the protostar. Here we present an analysis of radio observations obtained with the Very Large Array of the triple radio source in the Serpens star-forming region. This object is known to be a radio jet arising from an intermediate-mass protostar. It is also one of the first protostellar jets where the presence of nonthermal emission was proposed. We analyze the dynamics of the jet and the nature of the emission and discuss these issues in the context of the physical parameters of the jet and the particle acceleration phenomenon.
publishDate 2016
dc.date.none.fl_str_mv 2016-02-04
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
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://hdl.handle.net/11336/183020
Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Torrelles, Jose M.; Anglada, Guillem; et al.; Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens; IOP Publishing; Astrophysical Journal; 818; 1; 4-2-2016; 1-25
0004-637X
1538-4357
CONICET Digital
CONICET
url http://hdl.handle.net/11336/183020
identifier_str_mv Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Torrelles, Jose M.; Anglada, Guillem; et al.; Investigating particle acceleration in Protostellar Jets: The triple radio continuum source in serpens; IOP Publishing; Astrophysical Journal; 818; 1; 4-2-2016; 1-25
0004-637X
1538-4357
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://iopscience.iop.org/article/10.3847/0004-637X/818/1/27
info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/818/1/27
dc.rights.none.fl_str_mv 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
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv 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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score 13.070432

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