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A likely inverse-Compton emission from the Type IIb SN 2013df
DOI: 10.1038/srep30638
Bibcode: 2016NatSR...630638L
Kong, A. K. H.; Li, K. L.
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 a hard X-ray source that is associated with a Typ…
2016
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Scientific Reports
XMM-Newton
eHST
0