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Fig. 2

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Evolutionary tracks of a non-rotating 60 M star at Z = 0.014. The track with effective temperatures computed using our revised procedure (Teff,CMF) is shown in red, while previous estimates using the Geneva code are shown in dashed black (Teff,GVA; not corrected for the wind optical depth) and blue (Teff,GVAcorr; corrected for the wind optical depth). The filled circles correspond to timesteps for which a CMFGEN model was computed.

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