Fig. 10
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Projected rotational velocity distribution in the SMC (left), LMC (middle), and the Galaxy (right). The blue, purple, and green histograms corresponds to the XShootU plus complementary samples. The grey histograms show the 06–9.5 V-II stars of Mokiem et al. (2006) in the SMC, Ramírez-Agudelo et al. (2013) in the LMC, and of Holgado et al. (2022) in the Galaxy. The inserts in each panel show the cumulative distribution functions.
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