We investigate the capability of detecting, with Simbol-X, non-thermal
emission during stellar flares, and distinguishing it from hot thermal
emission. 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. Therefore
Simbol-X will detect the non-thermal emission from some of the X-ray brightest
nearby stars, whether the thermal vs. non-thermal relation, derived for solar
flares, holds.Comment: 2 pages, 2 postscript figures, proceedings of the workshop "Simbol-X:
the hard X-ray universe in focus", to be published in "Memorie of the Italian
Astronomical Society