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Fig. 16

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Edge-on view of the detected corrugation using the young giant sample. Left columns : vertical spatial residuals ΔZ as a function of galactocentric radius, R, for different slices in Galactic azimuth φ, as indicated by the individual labels. Points are colour-coded by the residuals in the vertical velocity ΔVZ. Black arrows show the direction and magnitude of the median residual vertical velocity ΔVZ. Right columns : same as left, but colour-coded by the median radial velocity VR. Black arrows show the direction and magnitude of the median radial velocity VR.

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