Figure 5 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.

Caption: Figure 5.

Distributions of the measured OH 35 (a) integrated fluxes and (b) equivalent widths.