Fig. 8

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Left: posterior probability distributions of infall velocity, Vin, peak optical depth, τ0, velocity dispersion, σ, excitation temperature of the “front” layer, Tf, and excitation temperature of the “rear” layer, Tr for the 37.7 GHz CH3OH transitiontowards W31C. The maximum posterior possibility point in the parameter space is shown in orange lines and points. The contours represent the 0.5, 1.0, 1.5, and 2.0σ confidence intervals. Right: observed and modelled spectra for the 37.7 GHz CH3OH transition. The blue spectrum represents the observed data, and the red curve indicates the fitted line from the two-layer model (see Sect. 4.1). The vertical black dashed line represents the systemic velocity of VLSR = −3.43 km s−1.
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