Image Details
Caption: Figure 11.
Detection rates of CO, H2O, HCN, C2H2, CO2, and OH for K and M stars in this sample of MRS spectra. Hatches show IRS or ground-based (for CO) detection rates from K. M. Pontoppidan et al. (2010). Earlier spectral types are excluded from this plot due to low number statistics in the JDISCS sample.
© 2025. The Author(s). Published by the American Astronomical Society.