Radio counterparts for gamma-ray sources

The latest generation of telescopes designed for the detection of high and very high energy gamma-rays have brought an enormous impulse to the research in this extreme portion of the electromagnetic spectrum. However, the astrophysical processes that give origin to emission at such high energies are...

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Detalles Bibliográficos
Autor principal: Dubner, G.
Formato: CONF
Materias:
Gamma-ray sources
Gamma-ray sources individual AGL 2021+4029
Radio Astronomy
Supernova Remnants
Supernova Remnants:individual G0.9+0.1
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0094243X_v1085_n_p195_Dubner
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_0094243X_v1085_n_p195_Dubner
record_format dspace
spelling todo:paper_0094243X_v1085_n_p195_Dubner2023-10-03T14:55:56Z Radio counterparts for gamma-ray sources Dubner, G. Gamma-ray sources Gamma-ray sources individual AGL 2021+4029 Radio Astronomy Supernova Remnants Supernova Remnants:individual G0.9+0.1 The latest generation of telescopes designed for the detection of high and very high energy gamma-rays have brought an enormous impulse to the research in this extreme portion of the electromagnetic spectrum. However, the astrophysical processes that give origin to emission at such high energies are still matter of debate. The search for counterparts in other spectral regimes, particularly in radio wavelengths, is a very useful tool to advance in the comprehension of the underlying physics. This contribution summarizes the characteristics of the best public radio databases and discusses the potential of dedicated high quality observations to investigate high-energy sources. © 2009 American Institute of Physics. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0094243X_v1085_n_p195_Dubner
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Gamma-ray sources
Gamma-ray sources individual AGL 2021+4029
Radio Astronomy
Supernova Remnants
Supernova Remnants:individual G0.9+0.1
spellingShingle Gamma-ray sources
Gamma-ray sources individual AGL 2021+4029
Radio Astronomy
Supernova Remnants
Supernova Remnants:individual G0.9+0.1
Dubner, G.
Radio counterparts for gamma-ray sources
topic_facet Gamma-ray sources
Gamma-ray sources individual AGL 2021+4029
Radio Astronomy
Supernova Remnants
Supernova Remnants:individual G0.9+0.1
description The latest generation of telescopes designed for the detection of high and very high energy gamma-rays have brought an enormous impulse to the research in this extreme portion of the electromagnetic spectrum. However, the astrophysical processes that give origin to emission at such high energies are still matter of debate. The search for counterparts in other spectral regimes, particularly in radio wavelengths, is a very useful tool to advance in the comprehension of the underlying physics. This contribution summarizes the characteristics of the best public radio databases and discusses the potential of dedicated high quality observations to investigate high-energy sources. © 2009 American Institute of Physics.
format CONF
author Dubner, G.
author_facet Dubner, G.
author_sort Dubner, G.
title Radio counterparts for gamma-ray sources
title_short Radio counterparts for gamma-ray sources
title_full Radio counterparts for gamma-ray sources
title_fullStr Radio counterparts for gamma-ray sources
title_full_unstemmed Radio counterparts for gamma-ray sources
title_sort radio counterparts for gamma-ray sources
url http://hdl.handle.net/20.500.12110/paper_0094243X_v1085_n_p195_Dubner
work_keys_str_mv AT dubnerg radiocounterpartsforgammaraysources
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