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We investigate the capability of detecting, with Simbol-X, non-thermalemission during stellar flares, and distinguishing it from hot thermalemission. We find that flare non-thermal emission is detectable when at least~20 cts are detected with the CZT detector in the 20-80 keV band. ThereforeSimbol-X will detect the non-thermal emission from some of the X-ray brightestnearby stars, whether the thermal vs. non-thermal relation, derived for solarflares, holds.

Simbol-X capability of detecting the non-thermal emission of stellar flares