The shadow over the southern half of the V1098 Sco protoplanetary disk is best explained by a misaligned inner disk, with rotation axes of the inner and outer disks separated by 38 degrees.
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Radiative Transfer Modeling of a Shadowed Protoplanetary Disk assisted by a Neural Network
The shadow over the southern half of the V1098 Sco protoplanetary disk is best explained by a misaligned inner disk, with rotation axes of the inner and outer disks separated by 38 degrees.