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Fig. A.1.
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Spectral evolution for models rs100/v1e4/b0p04 (top left), rs50/v1e4/b0p04 (top right), rs20/v1e4/b0p04 (bottom left), and rs10/v1e4/b0p04 (bottom right). The main difference between these models is the red-giant star radius (100, 50, 20, and 10 R⊙, given in the same order).
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