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Fig. 1


Evolutionary tracks of stars initially rotating with an equatorial velocity of ~ 100  km s-1, with initial masses in the range 10 M...100 M, in the HR diagram (left), and in the g − Teff diagram (right). The initial composition of the models is solar. The models up to 60 M are published by Brott et al. (2011), while those of higher mass are unpublished additions with identical input physics.

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