Seismic probing of the first dredge-up event through the eccentric red-giant and red-giant spectroscopic binary KIC 9163796 - How different are red-giant stars with a mass ratio of ~1.015?

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Fig. 13

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Total oscillation amplitudes for the extended sample of red giants (Kallinger et al. 2014), with their seismic mass colour-coded. The bulk of red dots on the left hand side mark secondary-clump stars. The measured and intrinsic amplitude of the primary component of KIC 9163796 are shown as the marker with error bars and the black framed diamond symbol, respectively.

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