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Fig. 10

image

υmacro as a function of log(ℒ / ℒ), with , for the sub-set of SMC B-type stars from Dufton et al. (2006; blue circles) and Galactic B-type stars from Simón-Díaz (2015; red circles) in the effective temperature range Teff17−23 kK, superposed on the computed (red continuous line for the MW, blue dashed for the SMC) as a function of log(ℒ / ℒ) at Teff = 20 kK.

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