Image Details
Caption: Figure 7.
The frequency of CEMP stars (with [C/Fe] > 0.7 or [C/Fe] > 1.0) as a function of metallicity (shown in green and blue, respectively). The low-mass AEOS stars are shown as a line, and observations from V. M. Placco et al. (2014) are shown as diamonds.
© 2025. The Author(s). Published by the American Astronomical Society.