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Fig. 8


Highest ratio of turbulent-to-total pressure in the envelopes of three 40Mstellar models with MW (red, continuous line), LMC (green, dashed line), and SMC (blue, dot-dashed line) metallicity as a function of effective temperature throughout part of their evolution. The scale on the right indicates the expected macroturbulent velocities () derived from the linear relation in Fig. 5 of Grassitelli et al. (2015a).

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