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- W58622085 abstract "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." @default.
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- W58622085 date "2001-12-01" @default.
- W58622085 modified "2023-09-23" @default.
- W58622085 title "Numerical Simulation of a Protostar Flare Loop between the Core and Disk" @default.
- W58622085 doi "https://doi.org/10.5303/jkas.2001.34.4.337" @default.
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