Fine-structure-resolved Rovibrational Excitation of OH due to Collisions with H<sub>2</sub> and He
POSTER
Abstract
We also present rate coefficients for vibrational transitions of OH due to He. Quasiresonant vibration-rotation transitions for relatively large rotational states near j=35.5 are discussed. In some cases, vibrationally inelastic cross-sections dominate over pure rotational transitions.
The calculations presented here are motivated by recent observations from the James Webb Space Telescope, which include spectra corresponding to the fundamental OH rovibrational band. State-to-state collisional rate coefficients with abundant perturbers are needed to interpret spectra taken from non-local thermodynamic equilibrium environments.
Publication: T.J. Price, Brandon Vargo, Caleb Taylor, Josiah Taylor, Robert C. Forrey, N. Balakrishnan, Zizhe Hu, B.H. Yang, and P.C. Stancil, "Fine-structure-resolved Rovibrational Excitation of OH due to Collisions with He for Non-Equilibrium Emission Modeling", (Manuscript in Preparation. To be submitted to ApJ)
Presenters
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T. J. J Price
Alvernia University
Authors
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T. J. J Price
Alvernia University
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Zizhe Hu
University of Georgia, Athens, GA 30602
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Benhui Yang
University of Georgia
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Konrad Patkowski
Auburn University, Auburn, AL 36849, Department of Chemistry and Biochemistry, Auburn University, Auburn, Alabama 36849, USA
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N. Balakrishnan
University of Nevada, Las Vegas, University of Nevada, Las Vegas, NV 89154
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Phillip C Stancil
University of Georgia
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Robert C Forrey
Penn State Berks