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Fig. 28


Escape probability for a photon to pass through 3500 km s-1 of core material (model 13G), at 100 (left), 200 (middle), and 400 (right) days (black). Also plotted are escape probabilities with respect to passage through the Fe/Co/He and Si/S clumps (red) and the O/Si/S, O/Ne/Mg, and O/C clumps (blue).

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