Fig. 3.
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Evolution of the interior atmospheric structure of the continuum optical depth (top) and the total Rosseland mean opacity (bottom) of a nonrotating 150 M⊙ star during the MS. The dashed red line shows the location of τ = 20, and the dashed black line marks a local density of 10−7 g cm−3. These represent the connection boundary for the atmosphere models outlined in Sect. 3.2.
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