Image Details
Caption: Figure 14.
Retrieved temperatures from C2H2 (left), HCN (middle), and CO2 (right) vs. the median emitting masses measured from the best-fit slab models for each disk, with marker styles indicating the submillimeter dust substructures listed in Table 2. No significant correlations are observed for C2H2 or HCN (Spearman ρ = −0.1, −0.04; p = 0.6, 0.8), but we report a significant negative correlation between CO2 temperature and emitting mass (Spearman ρ = −0.55; p = 0.02).
© 2025. The Author(s). Published by the American Astronomical Society.