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

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dc.creatorArgiroffi, C.
dc.creatorMicela, G.
dc.creatorMaggio, A.
dc.date2008-01-16
dc.date.accessioned2026-07-07T08:54:53Z
dc.date.available2026-07-07T08:54:53Z
dc.descriptionWe 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.
dc.description2 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"
dc.identifierhttps://arxiv.org/abs/0801.2532
dc.identifierhttp://arxiv.org/abs/0801.2532
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/146098
dc.subjectAstrophysics
dc.titleSimbol-X capability of detecting the non-thermal emission of stellar flares
dc.typetext

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