In the rebrightening of MAXI J1820+070, optical/UV emission is jet-dominated, and Balmer line profiles show the irradiated disk's inner radius shrinking from about 2e5 to 1e5 gravitational radii.
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Evolution of Accretion Disk Structure of the Black Hole X-ray Binary MAXI J1820$+$070 during the Rebrightening Phase
In the rebrightening of MAXI J1820+070, optical/UV emission is jet-dominated, and Balmer line profiles show the irradiated disk's inner radius shrinking from about 2e5 to 1e5 gravitational radii.