The accretion disk around the gainer in OGLE-LMC-DPV-062 varies mainly in vertical thickness over a 230-day cycle, with mass-transfer rate peaking at minimum light and inner edge obscuring more of the star.
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Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062
The accretion disk around the gainer in OGLE-LMC-DPV-062 varies mainly in vertical thickness over a 230-day cycle, with mass-transfer rate peaking at minimum light and inner edge obscuring more of the star.