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Fig. 3.

image

Hertzsprung–Russell diagram showing the terminal-age main sequence (TAMS) lines emerging from model grids computed with different combinations of overshooting αov and initial rotation velocity vrot, i (in units of km s−1). The semiconvective mixing efficiency is fixed to αsc = 1, but the TAMS-lines are insensitive to this parameter. The black lines indicate the corresponding zero age main sequences.

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