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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

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Sturm,  Eckhard
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Stone, M., Veilleux, S., González-Alfonso, E., Spoon, H., & Sturm, E. (2018). Constraints on the OH-to-H abundance ratio in infrared-bright galaxies derived from the strength of the OH 35 μm absorption feature. The Astrophysical Journal, 853(2): 132. doi:10.3847/1538-4357/aaa3df.


Cite as: https://hdl.handle.net/21.11116/0000-0000-AD17-4
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