The Influence of Magnetic Field on Accretion Disk Evaporation

Physics

Scientific paper

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Scientific paper

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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