Fig. 17
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Predicted Z coordinate (blue) and VZ pattern (red) as a function of Galactictocentric radius R based on the simple toy model described in Appendix D (see Equation (D.2)). The curves show the case of a corrugation propagating towards the outer parts of the disc at vc=10 km/s (left panel) or the inner parts of the disc at vc = −10 km/s (right panel).
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