Panel A: mass evolution over 4 Myr for a 85 M⊙ (solid line) and a 120 M⊙ star (dotted line) from literature data (Meynet & Maeder 2003). The dashed line shows a 100 M⊙ star interpolated from the two models. Panel B: luminosity evolution over 4 Myr for the same three stars as in the panel A. Panel C: radius evolution over 4 Myr for the same three stars as in panel A. Panel D: effective temperature evolution over 4 Myr for the same three stars as in panel A.
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