Numerical Simulation of a Protostar Flare Loop between the Core and Disk

Details Numerical Simulation of a Protostar Flare Loop between the Core and Disk Numerical Simulation of a Protostar Flare Loop between the Core and Disk

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jkas...34..337i&link_type=abstract

Journal of the Korean Astronomical Society, vol. 34, no. 4, pp. 337-339

Astronomy and Astrophysics

Astronomy

1

Methods: Numerical, Hydrodynamics, Stars: Flare

Scientific paper

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.

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