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Fig. 1


Temperature (panel a)) and density b) as a function of radius for a non-rotating star with initial mass of 60 M at metallicity Z = 0.014 for a O I model at stage 3 (as defined in Sect. 4). The solution obtained by the Geneva code is shown in black, while the final CMFGEN solution is displayed in solid red. A one-iteration CMFGEN solution used for initial guessing of the T structure is shown by the dashed blue line. A zoom-in on the connecting region of the Geneva and CMFGEN solutions (at τRoss = 10) is shown in the inset. The temperature and density structures of a model at stage 48 (WC) is displayed in panels c) and d), respectively.

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