arXiv · 0808.4006
Non-thermal emission from supernova shock breakout and the origin of the X-ray transient associated with SN2008D
Abstract
We suggest that non-thermal emission can be produced by multiple scatterings of the photons between the supernova ejecta and pre-shock material in supernova shock breakout. Such bulk-Comptonization process may significantly change the original thermal photon spectrum, forming a power-law non-thermal component at higher energies. We then show that the luminous X-ray outburst XRO081009 associated with SN2008D is likely to be such shock breakout emission from an ordinary type Ib/c supernova.
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Xiang-Yu Wang, Zhuo Li, Eli Waxman, Peter Meszaros. 2008-08-29. Non-thermal emission from supernova shock breakout and the origin of the X-ray transient associated with SN2008D. https://doi.org/10.1063/1.3027929
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