An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
Different types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medi...
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| Autores principales: | Supanitsky, A.D., De Souza, V. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14757516_v2013_n12_p_Supanitsky |
| Aporte de: |
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