Fig. 13.

Comparison of H I–H2 transition theory predictions with observations. Top panel: derived probability distribution function of αG from excitation of C I fine-structure levels. The green shaded region shows the interval estimate on αG corresponding to 0.683 confidence level. Bottom panel: theoretical H I surface density of a single H I–H2 transition layer as a function of αG Eq. (5) for shown by a solid blue line. The two dashed blue lines correspond to the derived range for
. The observed total H I column density is shown as a red horizontal line with downwards arrows, since part of the H I is likely not to be associated with the molecular cloud.
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