A Simulation of Flares in YSOs with Non-thermal Heating and Expected Hard X-ray Spectrum

Details A Simulation of Flares in YSOs with Non-thermal Heating and Expected Hard X-ray Spectrum A Simulation of Flares in YSOs with Non-thermal Heating and Expected Hard X-ray Spectrum

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..505k&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

We performed a one-dimensional hydrodynamic simulation of YSO flare loops, applying the flare mechanism for the sun. We assumed a flare loop connecting the central star and accretion disk. We found that the hard X-ray spectrum expected from our simulation has a very similar shape to the solar one obserbed by RHESSI, except that the energy band was 10 times higher than that of the solar flare.

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