Fig. 8.
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HRD of NGC 6791, with stars observed by Kepler coloured according to νmax. The inset zoomed-in views show the RGBb stars, including the four stars for which we have νmax values from Kepler. The orange and blue lines correspond to the evolutionary tracks with αMLT = 2.090 and αMLT = 2.290, respectively, and no envelope overshooting.
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