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Fig. A.3

image

Toppanels: reflex proper motions of individual galaxies in mas yr−1 as a function of the distance in arcmin to the center of 47 Tuc. The red solid line marks the running mean of the distribution. The left-hand panel shows the proper motion in the RA direction, whereas the right-hand panel is for the Dec direction. Bottom panels: same as the top panels but now for the proper motions of the cluster stars.

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