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Fig. 11

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Spectroscopic versus evolutionary masses. The red filled squares show the rotators with vsin   i ≥ 300 km s-1 (see text). Green symbols indicate masses as determined in Mokiem et al. (2006) for the stars in common with the present study. MPG 355 is not plotted because its evolutionary mass could not be determined with the model grid we used (Brott et al. 2011a).

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