Fig. 4

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Transformed radius (Rt) vs. T*. Models with Rt<200 R⊙ are in the dense-wind regime, i.e., with higher Ṁ and optical spectra crowded with emission and P Cygni features (shaded region). The colored texts in the lower part of the diagram name the wind-solution regions identified in the T* sequence. The 1-BiSJ and the 2-BiSJ are indicated by the dotted and dashed lines in the transitions from a valley to a plateau (i.e., increase in Ṁ) toward lower T*.
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