Fig. 13.
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Distributions of the magnitude of the galactocentric tangential velocity |vϑ| for HVSs that have traveled in DM halos with qz = {1.4, 1.0, 0.7}, and with qy = 0.7 (left panel) and qy = 1.4 (right panel). The distributions were generated with the same initial conditions (mock catalogs A) to highlight the effect of the different geometries of the DM halo.
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