Fig. 9.
Proper motion map (top) and residual proper motion map (bottom) of the Magellanic Bridge using Gaia DR2 proper motions for bins of stars with StarHorse distances > 30 kpc (black arrows). The median proper motion of the foreground Milky Way stars (with distances < 30 kpc) and the median proper motion of the Magellanic Bridge are indicated (blue and purple arrows, respectively).
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