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Cited article:

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CONSTRAINING THE MAGNETIC FIELD IN THE ACCRETION FLOW OF LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI

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THE DISK EVAPORATION MODEL FOR THE SPECTRAL FEATURES OF LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI

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The Spectral Features of Disk and Corona with Mass Evaporation in the Low/Hard State

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The rms-flux relation of Cyg X-2 in the horizontal branch

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Disk Evaporation–Fed Corona: Structure and Evaporation Features with Magnetic Field

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