Tales of stellar and binary coevolution, told by stellar oscillations - Binary demographics and their impact on stellar mass, orbits, and age estimates in main-sequence and red-giant stars

Open Access

Fig. 2.

Normalized kernel density estimates of the distributions for the stellar mass (left) and metallicity (right) for the APOKASC 3 (light) APO-K2 (dark) samples. The dots and vertical bars mark the respective sample’s median and the interquartile range (25^th–75^th percentiles). The dashed magenta line indicates the mass threshold of 1.8 M_⊙.

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