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Paper: The Influence of Magnetic Field on Accretion Disk Evaporation
Volume: 373, The Central Engine of Active Galactic Nuclei
Page: 139
Authors: Qian, L.; Liu, B.F.; Wu, X.-B.
Abstract: We numerically calculate the accretion disk coronal structure with different magnetic pressure and different heat conduction coefficients to obtain the evaporation rate-radius relation of X-ray binaries and AGN. We find that the truncation of the thin disk occurs at a smaller radius when the magnetic pressure is enhanced and the heat conduction is reduced.
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