Fig. 1
Domain of interest in (Teff,log g)-space. The filled circles are loci of the O-star MRL models with Z/Z⊙ ∈ (1/30,2) reported in L12. The open circles are the loci of models with Z/Z⊙ = 1/5 reported in this paper. The Eddington limit for static radiative envelopes is shown as well as H-burning evolutionary tracks (Brott et al. 2011) for masses 25 and 60 ℳ⊙.
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