Fig. 10.

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HRD of the single stars (gray points) with plotted on top the location of the overmassive stars in the RGB phase. The circles diamonds mark primary stars in a binary that are overmassive, while crosses indicate the overmassive lone primaries. The color represents the current mass of each overmassive star, and empty markers indicate the ones where detection of oscillations is not likely (P < 0.9).
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