Rotation-curve measurements of 15 protoplanetary disks show that the majority of dust rings and gaps sit at gas pressure maxima and minima, supporting pressure-driven dust trapping.
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exoALMA. VI. Rotating under Pressure: Rotation curves, azimuthal velocity substructures, and pressure variations
Rotation-curve measurements of 15 protoplanetary disks show that the majority of dust rings and gaps sit at gas pressure maxima and minima, supporting pressure-driven dust trapping.