Physical conditions in the gas phases of the giant H II region LMC-N 11 - II. Origin of [C II] and fraction of CO-dark gas

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Fig. 14

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Same as Fig. 9 but with the total molecular gas fraction (i.e., including the CO-dark H₂ gas). The vertical striping is due to the wide ranges for the molecular gas fraction determination for the faintest [C II] components. The shade scales with the density of points.

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