Figure 14 from Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

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Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

Authors: Lucas S. Viani, and Sarbani Basu

2020 The Astrophysical Journal 904 22.

Provider: AAS Journals

Caption: Figure 14.

Likelihood weighted average of the input overshoot value (in units of H_P) plotted as a function of a variety of stellar properties for the stars in the study. The red line is a weighted linear best fit.

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