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Optical and X-ray Afterglows in the Cannonball Model of GRBs
The Cannonball Model is based on the hypothesis that GRBs and their afterglows are made in supernova explosions by relativistic ejecta similar to the ones observed in quasars and microquasars. Its predictions are simple, and analytical in fair approximations. The model describes well the properties...
Autor principal: | De Rújula, Alvaro |
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Lenguaje: | eng |
Publicado: |
2002
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1063/1.1579367 http://cds.cern.ch/record/534632 |
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