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Fig. 22


Evolution of the equatorial rotational velocity as a function of time for the stellar evolution models calculated by Brott et al. (2011, solid lines) and a 60 M track (dashed line) published by Meynet & Maeder (2005). Both studies account for very rapid rotation (vrot,ini> 500 km s-1) and an initial metallicity of 0.14 Z. The labels close to the tracks refer to the initial mass. The color coding is the same as in Figs. 18 and 19 (see also the inlet).

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