Fig. 11.
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Gaia EDR3 proper motion maps of the LMC for samples of stars < 1 Gyr old (top) and > 2 Gyr old (bottom) (see text for details). Each vector represents the median proper motion of at least 100 stars for the young population and of at least 2000 stars for the old population. The central vector indicates the bulk motion of the LMC as shown in Fig. 9.
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