Fig. 11.
Proper motions μδ and μα cos δ for the sample of stars selected based on StarHorse distances (> 30 kpc). Proper motions of VMC (blue triangles), Gaia DR2 (red squares), N-body particles (grey dots), HST measurements (black squares) and the GalMod Milky Way foreground (empty circles) are shown as a function of projected distance from the SMC centre.
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