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Fig. 16
Comparison of the observed evolution of equatorial velocity ratios in the MS life time span for stars with M = 3 M⊙ inferred from observations with theoretical ones calculated by Ekström et al. (2008) for different v/vcrit on the ZAMS. a) Evolution of ⟨ v/vcrit ⟩ ratios; b) evolution of ⟨ v/vZAMS ⟩ ratios.
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