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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2009
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1085_n_p195_Dubner http://hdl.handle.net/20.500.12110/paper_0094243X_v1085_n_p195_Dubner |
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paper:paper_0094243X_v1085_n_p195_Dubner2023-06-08T15:09:04Z Radio counterparts for gamma-ray sources 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. 2009 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1085_n_p195_Dubner 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 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. |
| 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 |
| publishDate |
2009 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1085_n_p195_Dubner http://hdl.handle.net/20.500.12110/paper_0094243X_v1085_n_p195_Dubner |
| _version_ |
1768544172270157824 |