Fig. 6
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Time sequences of bolometric surface intensity for the large 1 M⊙ model st28gm06n052 (snapshots about 8 and 14 months apart, see the counter at the top of the panels) and the 1.5 M⊙ model st28gm05n033 (snapshots about 3.5 and 7 months apart). Only the inner part of computational box that contains the star is plotted, on the same scale for both models.
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