Open Access

Fig. 13

image

log (N/C) vs. logg for the sample stars. The evolutionary tracks are labelled by initial mass. Full lines show models with initial rotation vinit = 0.4vcrit, dot-dashed and dashed lines show models with vinit = 0.1vcrit and 0.2vcrit, respectively. Left: stars less massive than the average mass of the sample, i.e. 30 M. Stars rotating faster than 200 km s−1 are highlighted by thick black circles. Right: stars with initial masses above the average for the whole sample. See text for more details

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