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Numerical Simulation of a Protostar Flare Loop between the Core and Disk
ISOBE HIROAKI,YOKOYAMA TAKAAKI,SHIBATA KAZUNARI The Korean Astronomical Society 2001 Journal of The Korean Astronomical Society Vol.34 No.4
One-dimensional hydrodynamic modeling of a protostellar flare loop is presented. The model consists of thermally isolated loop connecting the central core and the accretion disk. We found that the conductive heat flux of a flare heated the accretion disk up to coronal temperature and consequently the disk is evaporated and disappeard. This effect may explain the ovserved feature of the repeated flare from the young stellar object YLW 15.