Fig. 19
Comparing the eccentricities of known eccentric systems with ellipsoidal modulation. Colour indicates the log g of the red giant component. Dots represent the stars from our sample for which we could derive the eccentricities from radial velocities. KIC 5006817 and KIC 8410637 are shown as a cross and triangle, respectively. Squares show the derived eccentricities of the stars in the LMC.
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