The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission
- Autores
- Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Romero, Gustavo Esteban; Torrelles, José M.; Rodríguez, Luis F.; Anglada, Guillem; Martí, Josep; Perucho, Manel; Valotto, Carlos Alberto
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that nonthermal emission could also be present. This additional contribution from nonthermal emission has been inferred through negative spectral indices at centimeter wavelengths in some regions of the radio jets. In the case of HH 80-81, one of the most powerful protostellar jets known, linearly polarized emission has also been detected, revealing that the nonthermal emission is of synchrotron nature from a population of relativistic particles in the jet. This result implies that an acceleration mechanism should be taking place in some parts of the jet. Here, we present new high sensitivity and high angular resolution radio observations at several wavelengths (in the 3-20 cm range) of the HH 80-81 radio jet. These new observations represent an improvement in sensitivity and angular resolution by a factor of ∼10 with respect to previous observations. This allows us to resolve the morphology of the radio jet and to study the different emission mechanisms involved through spectral index maps. We conclude that synchrotron emission in this jet arises from an extended component detected at low frequencies and from the termination points of the jet, where strong shocks against the ambient medium can produce efficient particle acceleration.
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. Instituto de Radioastronomía y Astrofísica; México
Fil: Carrasco Gonzalez, Carlos Eugenio. Instituto de Radioastronomía y Astrofísica; México
Fil: Araudo, Anabella Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Astronomical Institute of the Academy of Sciences; República Checa
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: Torrelles, José M.. Consejo Superior de Investigaciones Científicas; España
Fil: Rodríguez, Luis F.. Instituto de Radioastronomía y Astrofísica; México
Fil: Anglada, Guillem. Consejo Superior de Investigaciones Científicas; España
Fil: Martí, Josep. Universidad de Jaén; España
Fil: Perucho, Manel. Universidad de Valencia; España
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
STARS: FORMATION - 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:11336/64850
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The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal EmissionRodríguez Kamenetzky, Adriana RaquelCarrasco Gonzalez, Carlos EugenioAraudo, Anabella TeresaRomero, Gustavo EstebanTorrelles, José M.Rodríguez, Luis F.Anglada, GuillemMartí, JosepPerucho, ManelValotto, Carlos AlbertoACCELERATION OF PARTICLESISM: JETS AND OUTFLOWSSTARS: FORMATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that nonthermal emission could also be present. This additional contribution from nonthermal emission has been inferred through negative spectral indices at centimeter wavelengths in some regions of the radio jets. In the case of HH 80-81, one of the most powerful protostellar jets known, linearly polarized emission has also been detected, revealing that the nonthermal emission is of synchrotron nature from a population of relativistic particles in the jet. This result implies that an acceleration mechanism should be taking place in some parts of the jet. Here, we present new high sensitivity and high angular resolution radio observations at several wavelengths (in the 3-20 cm range) of the HH 80-81 radio jet. These new observations represent an improvement in sensitivity and angular resolution by a factor of ∼10 with respect to previous observations. This allows us to resolve the morphology of the radio jet and to study the different emission mechanisms involved through spectral index maps. We conclude that synchrotron emission in this jet arises from an extended component detected at low frequencies and from the termination points of the jet, where strong shocks against the ambient medium can produce efficient particle acceleration.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. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Carrasco Gonzalez, Carlos Eugenio. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Araudo, Anabella Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Astronomical Institute of the Academy of Sciences; República ChecaFil: 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: Torrelles, José M.. Consejo Superior de Investigaciones Científicas; EspañaFil: Rodríguez, Luis F.. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Anglada, Guillem. Consejo Superior de Investigaciones Científicas; EspañaFil: Martí, Josep. Universidad de Jaén; EspañaFil: Perucho, Manel. Universidad de Valencia; EspañaFil: 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 Publishing2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/64850Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Romero, Gustavo Esteban; Torrelles, José M.; et al.; The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 1-160004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/reference/doi/10.3847/1538-4357/aa9895info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa9895info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1711.02554info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/aa9895info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:39:15Zoai:ri.conicet.gov.ar:11336/64850instacron: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 10:39:15.755CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
title |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
spellingShingle |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission Rodríguez Kamenetzky, Adriana Raquel ACCELERATION OF PARTICLES ISM: JETS AND OUTFLOWS STARS: FORMATION |
title_short |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
title_full |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
title_fullStr |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
title_full_unstemmed |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
title_sort |
The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission |
dc.creator.none.fl_str_mv |
Rodríguez Kamenetzky, Adriana Raquel Carrasco Gonzalez, Carlos Eugenio Araudo, Anabella Teresa Romero, Gustavo Esteban Torrelles, José M. Rodríguez, Luis F. Anglada, Guillem Martí, Josep Perucho, Manel Valotto, Carlos Alberto |
author |
Rodríguez Kamenetzky, Adriana Raquel |
author_facet |
Rodríguez Kamenetzky, Adriana Raquel Carrasco Gonzalez, Carlos Eugenio Araudo, Anabella Teresa Romero, Gustavo Esteban Torrelles, José M. Rodríguez, Luis F. Anglada, Guillem Martí, Josep Perucho, Manel Valotto, Carlos Alberto |
author_role |
author |
author2 |
Carrasco Gonzalez, Carlos Eugenio Araudo, Anabella Teresa Romero, Gustavo Esteban Torrelles, José M. Rodríguez, Luis F. Anglada, Guillem Martí, Josep Perucho, Manel Valotto, Carlos Alberto |
author2_role |
author author author author author author author author author |
dc.subject.none.fl_str_mv |
ACCELERATION OF PARTICLES ISM: JETS AND OUTFLOWS STARS: FORMATION |
topic |
ACCELERATION OF PARTICLES ISM: JETS AND OUTFLOWS STARS: FORMATION |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that nonthermal emission could also be present. This additional contribution from nonthermal emission has been inferred through negative spectral indices at centimeter wavelengths in some regions of the radio jets. In the case of HH 80-81, one of the most powerful protostellar jets known, linearly polarized emission has also been detected, revealing that the nonthermal emission is of synchrotron nature from a population of relativistic particles in the jet. This result implies that an acceleration mechanism should be taking place in some parts of the jet. Here, we present new high sensitivity and high angular resolution radio observations at several wavelengths (in the 3-20 cm range) of the HH 80-81 radio jet. These new observations represent an improvement in sensitivity and angular resolution by a factor of ∼10 with respect to previous observations. This allows us to resolve the morphology of the radio jet and to study the different emission mechanisms involved through spectral index maps. We conclude that synchrotron emission in this jet arises from an extended component detected at low frequencies and from the termination points of the jet, where strong shocks against the ambient medium can produce efficient particle acceleration. 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. Instituto de Radioastronomía y Astrofísica; México Fil: Carrasco Gonzalez, Carlos Eugenio. Instituto de Radioastronomía y Astrofísica; México Fil: Araudo, Anabella Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Astronomical Institute of the Academy of Sciences; República Checa 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: Torrelles, José M.. Consejo Superior de Investigaciones Científicas; España Fil: Rodríguez, Luis F.. Instituto de Radioastronomía y Astrofísica; México Fil: Anglada, Guillem. Consejo Superior de Investigaciones Científicas; España Fil: Martí, Josep. Universidad de Jaén; España Fil: Perucho, Manel. Universidad de Valencia; España 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 |
Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that nonthermal emission could also be present. This additional contribution from nonthermal emission has been inferred through negative spectral indices at centimeter wavelengths in some regions of the radio jets. In the case of HH 80-81, one of the most powerful protostellar jets known, linearly polarized emission has also been detected, revealing that the nonthermal emission is of synchrotron nature from a population of relativistic particles in the jet. This result implies that an acceleration mechanism should be taking place in some parts of the jet. Here, we present new high sensitivity and high angular resolution radio observations at several wavelengths (in the 3-20 cm range) of the HH 80-81 radio jet. These new observations represent an improvement in sensitivity and angular resolution by a factor of ∼10 with respect to previous observations. This allows us to resolve the morphology of the radio jet and to study the different emission mechanisms involved through spectral index maps. We conclude that synchrotron emission in this jet arises from an extended component detected at low frequencies and from the termination points of the jet, where strong shocks against the ambient medium can produce efficient particle acceleration. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-12 |
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/11336/64850 Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Romero, Gustavo Esteban; Torrelles, José M.; et al.; The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 1-16 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/64850 |
identifier_str_mv |
Rodríguez Kamenetzky, Adriana Raquel; Carrasco Gonzalez, Carlos Eugenio; Araudo, Anabella Teresa; Romero, Gustavo Esteban; Torrelles, José M.; et al.; The Highly Collimated Radio Jet of HH 80-81: Structure and Nonthermal Emission; IOP Publishing; Astrophysical Journal; 851; 1; 12-2017; 1-16 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/reference/doi/10.3847/1538-4357/aa9895 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/aa9895 info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1711.02554 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/aa9895 |
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 |
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 |