Fig. 7
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Hertzsprung-Russell diagram of XshootU sample (LMC: blue circles, SMC: green triangles), together with LMC evolutionary tracks for 10–200 M⊙ main-sequence stars from Brott et al. (2011) and Köhler et al. (2015). Evolutionary masses of post-main sequence stars are determined from TAMS luminosities of SMC tracks from Schootemeijer et al. (2019).
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