Highest ratio of turbulent-to-total pressure in stellar models at the effective temperature of Teff = 30 000 K, with MW (red, continuous line), LMC (green, dashed line), and SMC (blue, dot-dashed line) metallicity as a function of their luminosity. The scale on the right indicates the expected macroturbulent velocities () derived from the linear fit in Fig. 5 of Grassitelli et al. (2015a).
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