Fig. 9.

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Results on the absolute proper motions of LMC and SMC star clusters. Left: coordinates, in degrees, relative to the SMC center of the studied SMC and LMC clusters. The arrows in the top panel are indicative of the absolute proper motions of each cluster, while the bottom panel represents the proper motions of LMC and SMC clusters after subtracting the average motion of the corresponding galaxy. Right: proper motions of stars brighter than GBP = 16.0 mag in the region around the LMC and the SMC (black points). The studied LMC and SMC clusters are plotted in all panels with red and aqua dots, respectively.
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