Fig. 9
Rotation curves as a function of the height from the Milky Way mid-plane used in modelling. The thick lines on top stand for the mid-plane rotation. Red solid lines: receding curves; blue dashed lines: approaching curves; black dotted lines: rotation velocities assumed for the “shallow rise” model at R < 4.5 kpc. For R > 7.7 kpc we assumed that the curves are flat.
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