Open Access

Fig. 8

image

Evolution of the radius as a function of the mixed-mode density on the red giant branch. Coloured triangles represent the measurements obtained in this study, the colour coding represents the mass estimated from the asteroseismic global parameters. Evolutionary tracks are computed with MESA for different masses. The coloured dots indicate the bottom of the RGB for the different masses. The vertical black dashed line indicates the lower observational limit for the mixed-mode density, .

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