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Fig. 15

image

Relation of the SO (top row) and 34SO (bottom row) molecular abundances to cloud physical parameters: kinetic temperature (left), extinction (middle), and molecular hydrogen density (right). The dataset is color-coded according to the molecular cloud of the points, as indicated in the legend. Black lines show the linear correlations between molecular abundances and molecular hydrogen density for the corresponding whole samples, with the correlation parameters indicated in the legends.

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