Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202039465e]


Fig. 8

image

Posterior probability distributions of C18O column density, , rotational temperature, Trot, the C18O (1–0) opacity, τ18,1, and the C18O (2–1) opacity, τ18,2, toward the dense core, Bolo12, with the maximum posterior possibility point in the parameterspace shown in orange lines and points. Contours denote the 0.5, 1.0, 1.5, and 2.0σ confidence intervals.

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