Image Details
Caption: Figure 16.
Starspot isochrones at solar composition evaluated at 100 Myr, 300 Myr, and the ZAMS (defined where Xcen/Xcen,0 = 0.993); and 0% (solid), 25% (dashed), and 50% (dotted) spot filling factors. Mass tracks are shown for constituent tracks evolved to the ZAMS. The A. W. Mann et al. (2015) sample is overplotted with reported errors. Colors are assigned by the stellar mass, as shown in the color bar.
© 2026. The Author(s). Published by the American Astronomical Society.