Image Details
Caption: Figure 7.
Posterior distributions of the model parameters from the MCMC fit. Diagonal panels show marginalized one-dimensional posteriors; off-diagonal panels show two-dimensional projections that reveal covariances. The 12C/13C and 18O/17O ratios are tightly constrained and largely uncorrelated with other parameters, whereas 16O/18O and ﹩\mathrm{log}{N}_{{\rm{CO}}}﹩ exhibit strong covariance, reflecting the moderate optical depth of C18O(1–0).
© 2026. The Author(s). Published by the American Astronomical Society.