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Fig. 5
Mass-loss rates (left panel), wind speeds (middle panel) and mean degree of dust condensation near a “threshold” as function of luminosity. All other stellar parameters are kept the same (M ⋆ = 1 M⊙, Teff = 2600 K, log (C − O) = 8.80).
This figure is made of several images, please see below:
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