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A likely inverse-Compton emission from the Type IIb SN 2013df
The inverse-Compton X-ray emission model for supernovae has been well established to explain the X-ray properties of many supernovae for over 30 years. However, no observational case has yet been found to connect the X-rays with the optical lights as they should be. Here, we report the discovery of...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Nature Publishing Group
2016
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4969746/ https://www.ncbi.nlm.nih.gov/pubmed/27481538 http://dx.doi.org/10.1038/srep30638 |