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A schematic sketch of the evolution in star-disk interaction.
Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations
In numerical simulations of the star-disk system, after the relaxation, the disk is truncated at the truncation radius R_t. Position of the R_t is close to the line of balance of the disk ram pressure and the magnetic pressure, which is located between a central object and the disk inner radius.
Magnetospheric Accretion and Ejection of Matter in Resistive MHD Simulations
Chiang, Tzu-Yang
Assistant
photo of Chiang, Tzu-Yang
Office: ASMAB 1208
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Research Interests

Functional Analysis

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