Fig. 1
HR diagram showing the computed stellar evolution tracks. The colors of the dots indicate the maximum fraction of turbulent-to-total pressure occurring within the stellar envelopes (see framed color bar in the bottom left corner). Stellar models in red show Pturb/P> 10%. The masses of the models are indicated next to the tracks. For the upper HR diagram, see Fig. 1 in Grassitelli et al. (2015).
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