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Fig. 10


ΘRT vs. v sin i for the stars in where v sin i(FT) and v sin i(GOF) agree to better than 20%. Filled and dotted circles indicate the O- and B-type stars, respectively. The indicated values of ΘRT for all the stars with v sin i 180 km s-1 must be considered as upper limits. The regions in which v sin i and ΘRT measurements can be affected by the effect of microturbulent broadening (see text for explanation) are indicated in gray. Dashed and dotted lines indicate the 1:1, 2.2:1, and 1:0.5 relations, respectively.

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