Fig. 7
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Same as Fig. 6, but for a model sequence with log L/L⊙ = 5.475, M = 15 M⊙, and ХH = 0. Contrary to the situation in Fig. 6 for a 20 M⊙ star, there is an abrupt breakdown of solutions beyond a minimum temperature and a maximum Ṁ. For the T2/з- and Teff(τcrit)-scales these points are marked with a vertical line attached to a gray-hatched area.
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