Fig. 7.
Rotational velocity probability distributions, f(ve), for the apparently single B-type stars in NGC 346 deduced from the PF (black line) and FT (red line) estimates, and for the equivalent sample in 30 Doradus (dotted blue line) of Dufton et al. (2013). Also shown are the equivalent distributions for the apparently single Be-type (dash-dotted black and red lines).
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