Large optical modulations during 2018 outburst of MAXI J1820+070 reveal evolution of warped accretion disc through X-ray state change
Jessymol K. Thomas, Philip A. Charles, David A. H. Buckley, Marissa M., Kotze, Jean-Pierre Lasota, Stephen B. Potter, James F. Steiner, John A. Paice

TL;DR
This study analyzes optical, X-ray, and radio data from the 2018 outburst of MAXI J1820+07, revealing large optical modulations linked to a warp in the accretion disc that evolves during the state change.
Contribution
It provides the first detailed temporal analysis connecting optical modulations with disc warping and state transitions in a black-hole X-ray transient.
Findings
High amplitude optical modulations (>0.5 mag) evolve from superhump to orbital period.
Optical modulation peaks correlate with X-ray state transitions and jet ejections.
Warped disc geometry is driven by irradiation, affecting the observed modulations.
Abstract
The black-hole X-ray transient MAXI J1820+07 (=ASSASN-18ey) discovered in March 2018 was one of the optically brightest ever seen, which has resulted in very detailed optical outburst light-curves being obtained. We combine them here with X-ray and radio light-curves to show the major geometric changes the source undergoes. We present a detailed temporal analysis that reveals the presence of remarkably high amplitude (>0.5 mag) modulations, which evolve from the superhump (16.87 h) period towards the presumed orbital (16.45 h) period. These modulations appear ~87d after the outburst began, and follow the Swift/BAT hard X-ray light-curve, which peaks 4 days before the radio flare and jet ejection, when the source undergoes a rapid hard to soft state transition. The optical modulation then moves closer to the orbital period, with a light curve peak that drifts slowly in orbital phase from…
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