Image Details
Caption: Figure 4.
CMD of Boo I main-sequence member stars, overlaid with BaSTI α-enhanced isochrone (blue) and our O-enhanced isochrone (red), both having an age of 13.3 Gyr and [Fe/H] = −2.4, with labels indicating specific stellar masses. The red error bars indicate the typical photometric uncertainties at each magnitude.
© 2026. The Author(s). Published by the American Astronomical Society.