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Fig. 13.
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Evolution of averaged fluxes, gradients, and velocity for a 1 M⊙ stellar model with log10L/L⊙ = 0.0, log10Teff = 3.76 and solar metallicity. Left panel refers to R = 0.7 R⊙, right panel to R = 0.88 R⊙. Data are from Pasetto et al. (2019).
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