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• W3103967956 startingPage "881" @default.
• W3103967956 abstract "We investigate roles of the bulk comptonization process in the propagation of thermal photons emitted at the shock breakout of a supernova explosion. We use a hydrodynamical model based on a self-similar solution for the shock breakout. The propagation of photons is treated by a Monte-Carlo technique. Results of the simulations successfully reproduce the power-law spectrum observed by X-ray observations for XRF 080109/SN 2008D, if a mildly relativistic shock velocity is assumed. Effects of some radiative processes, photoionization, radiative recombination, and free-free absorption on the propagation of emitted photons are also investigated. It is found that none of them hardly changes the spectrum regarding the progenitor stars of type Ib or Ic supernovae. Light curves calculated under the assumption of a spherical explosion indicate that the progenitor radius is required to be $/sim 10^{13}$ cm." @default.
• W3103967956 created "2020-11-23" @default.
• W3103967956 creator A5021510532 @default.
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• W3103967956 date "2010-07-23" @default.
• W3103967956 modified "2023-10-06" @default.
• W3103967956 title "NON-THERMAL PHOTON PRODUCTION VIA BULK COMPTONIZATION AT SUPERNOVA SHOCK BREAKOUT" @default.
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• W3103967956 doi "https://doi.org/10.1088/0004-637x/719/1/881" @default.
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