Abstract
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.
| Lingua originale | English |
|---|---|
| Pagine | 219-220 |
| Numero di pagine | 2 |
| Stato di pubblicazione | Published - 2008 |