Fig. 1

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Kiel diagram showing the five different regions of model coverage (O, B1, B2, BSG1, and BSG2). Overlayed are Ekström et al. (2012) evolutionary tracks for rotating stars (vini/vcrit = 0.4) at solar metallicity (black lines) for different masses, as indicated. The five-pointed black stars mark the positions of the single stars analysed in the present work and the matching open symbols are the components in the analysed binary systems.
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