Fig. 13
Line source function of Brα (in units of the local Planck function) and velocity gradient (vertically scaled) as a function of τRoss, for the same Ṁ-sequence as in Fig. 12. Note that the transition region between photosphere and wind moves towards lower τRoss for decreasing Ṁ, i.e., the model with the lowest mass-loss is located at the right of the figure.
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