Figure 6 from Constraints on the OH-to-H Abundance Ratio in Infrared-bright Galaxies Derived from the Strength of the OH 35 μm Absorption Feature

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Constraints on the OH-to-H Abundance Ratio in Infrared-bright Galaxies Derived from the Strength of the OH 35 μm Absorption Feature

Authors: Myra Stone, Sylvain Veilleux, Eduardo González-Alfonso, Henrik Spoon, and Eckhard Sturm

2018 The Astrophysical Journal 853 132.

Provider: AAS Journals

Caption: Figure 6.

Distributions of the (a) OH column densities and (b) OH-to-H abundance ratios, ﹩{X}_{\mathrm{OH}}﹩, inferred from the fits of the OH 35 feature (assuming a gas-to-dust ratio of 125).

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