A 10-Jupiter-mass planet flying through a protoplanetary disk creates observable spiral arms that differ between prograde (two arms) and retrograde (one arm) encounters.
A., Price Daniel J., Pinte Christophe, Cuello Nicol \'a s
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Simulation of images of protoplanetary disks after collision with free-floating planets
A 10-Jupiter-mass planet flying through a protoplanetary disk creates observable spiral arms that differ between prograde (two arms) and retrograde (one arm) encounters.