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Paper: A Simulation of Flares in YSOs with Non-thermal Heating and Expected Hard X-ray Spectrum
Volume: 369, New Solar Physics with Solar-B Mission
Page: 505
Authors: Kawamichi, T.; Shibata, K.
Abstract: 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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