A disk cavity around a supermassive black hole binary is predicted to break the lag-wavelength relation into a flat short-wavelength part and a steeper long-wavelength part.
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Continuum Reverberation Mapping of Accretion Disks Surrounding Supermassive Black Hole Binaries: Observational Signatures
A disk cavity around a supermassive black hole binary is predicted to break the lag-wavelength relation into a flat short-wavelength part and a steeper long-wavelength part.