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We map the planetary wake associated with the embedded protoplanet creatingthe CO kink in the disk of HD~163296. We show that the wake can be traced by aseries of correlated perturbations in the peak velocity map. The sign change ofthe perturbations across the disk major axis confirm that the wake inducespredominantly radial motion, as predicted by models of planet-disk interaction.These results provide the first direct confirmation of planet wakes generatedby Lindblad resonances. Mapping the wake provides a constraint on the diskaspect ratio, which is required to measure the mass of the planet.

Mapping the Planetary Wake in HD 163296 with Kinematics