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Isotopic Ratios in the Disk of HD 163296

  • Authors: Chunhua Qi, David J. Wilner, Catherine C. Espaillat

Chunhua Qi et al 2026 The Astrophysical Journal Letters 997 .

  • Provider: AAS Journals

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).

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