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Electron Acceleration in Supernovae and Millimeter Perspectives
Supernovae launch a strong shock wave by the interaction of the expanding ejecta and surrounding circumstellar matter (CSM). At the shock, electrons are accelerated to relativistic speed, creating observed synchrotron emissions in radio wavelengths. In this paper, I suggest that SNe (i.e., <...
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| Autor principal: | |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
CTU Central Library
2014-12-01
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| Colecção: | Acta Polytechnica CTU Proceedings |
| Acesso em linha: | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2389 |
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