Figure 15 from Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 15.

Top: Input overshoot as a function of the a₁ coefficient for the sample of stars. Here, the a₁ value is determined from the observed frequencies of the stars. The red line is a weighted line of best fit. Bottom: Input overshoot as a function of the a₀ coefficient for the sample of stars. In both panels overshoot is in units of H_P.

Other Images in This Article

Copyright and Terms & Conditions