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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 7.

OH 35 spectra normalized to the continuum. Red and blue lines are the two Gaussian components of the fitted line, and the magenta line is the sum of the two components. The green line is the profile predicted by the radiative transfer model described in González-Alfonso & Cernicharo (1999) and González-Alfonso et al. (2017). The modeled line profiles are constrained by observations of 4 OH lines at 65, 79, 84, and 119 μm.

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