Image Details
Caption: Figure 19.
A comparison between full YREC rotation models and rotevol forward models for tracks with masses 0.6, 0.8, 1.0, and 1.2 M⊙. The upper panel shows the comparison between the predicted rotation periods under the solid-body approximation. The lower panel shows the difference in predicted rotation periods for non-solid-body rotation with core–envelope coupling timescales given by P. A. Denissenkov et al. (2010).
© 2026. The Author(s). Published by the American Astronomical Society.