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Fig. 6.
Positions of the stars with a determined υsin(i) taken from Simón-Díaz et al. (2017) and Holgado et al. (2020, and in prep.) in the spectroscopic HR diagram. The evolutionary tracks correspond to non-rotating tracks with an α = 0.3. The left-panel shows the mass selection and the right panel shows the υsin(i) distribution.
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