Fig. 3.
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Rotation profiles as a function of the Lagrangian mass at various stages of MS evolution (labeled by the central hydrogen content Xc) of three models. The dotted lines indicate a rotating 30 M⊙ single star S2. Dashed and solid lines indicate the primary star in B2 with initial Porb = 20.0 days and the primary star in B1 with initial Porb = 6.0, respectively.
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