Image Details
Caption: Figure 3.
The effects of core (top row) and envelope (bottom row) overshooting on evolutionary tracks of 2−8 M⊙ models of high (Z = 0.014, left column), intermediate (Z = 0.004, middle column), and low (Z = 0.0014, right column) metallicity. Fiducial hot IS strip is overplotted for a reference.
© 2026. The Author(s). Published by the American Astronomical Society.