High Energy Processes in Protostellar Jets

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...

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Autores principales: Rodríguez Kamenetzky, Adriana, Carrasco González, CAarlos, Araudo, Anabella Teresa, Torrelles, José María, Anglada, Guillem, Marti, Josep, Rodríguez, Luis Felipe, Valotto, Carlos
Formato: Objeto de conferencia
Lenguaje:Español
Publicado: 2015
Materias:
Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/168048
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-168048
record_format dspace
spelling I19-R120-10915-1680482024-07-22T20:01:58Z http://sedici.unlp.edu.ar/handle/10915/168048 High Energy Processes in Protostellar Jets Rodríguez Kamenetzky, Adriana Carrasco González, CAarlos Araudo, Anabella Teresa Torrelles, José María Anglada, Guillem Marti, Josep Rodríguez, Luis Felipe Valotto, Carlos 2015-10 2016 2024-07-22T17:09:11Z es Ciencias Astronómicas protostellar jets The Triple Radio Source in Serpens 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 Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 105-110
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
spellingShingle Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
Rodríguez Kamenetzky, Adriana
Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
High Energy Processes in Protostellar Jets
topic_facet Ciencias Astronómicas
protostellar jets
The Triple Radio Source in Serpens
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.
format Objeto de conferencia
Objeto de conferencia
author Rodríguez Kamenetzky, Adriana
Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
author_facet Rodríguez Kamenetzky, Adriana
Carrasco González, CAarlos
Araudo, Anabella Teresa
Torrelles, José María
Anglada, Guillem
Marti, Josep
Rodríguez, Luis Felipe
Valotto, Carlos
author_sort Rodríguez Kamenetzky, Adriana
title High Energy Processes in Protostellar Jets
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
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/168048
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