Presentation Information
[C08-5-03]General Relativistic Radiation Magnetohydrodynamical simulations of Super-Eddington Accretion Flows onto Magnetized Neutron Stars; Powerful Outflows and Thermal Emission
*Akihiro Inoue1, Ken Ohsuga1, Hiroyuki R. Takahashi2, Yuta Asahina1 (1. University of Tsukuba (Japan), 2. Komazawa University (Japan))
Keywords:
Neutron star,Magnetohydrodynamical simulation,general relativity,radiation,plasma physics
