Open Access
Fig. 13.
Median vertical velocity vz distribution on the Galactic plane. We divided the XY plane into bins of 200 pc width, and we only show the ones containing more than ten stars. The dashed circles have radii from 1 to 9 kpc, in steps of 1 kpc. The Galactic warp is visible for R > 4 kpc towards the Galactic anti-centre.
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