Formation of the Hydroxyl Radical by Radiative Association

Author:

Svensson S. Karl-Mikael1,Gustafsson Magnus2,Nyman Gunnar1

Affiliation:

1. Department of Chemistry and Molecular Biology, University of Gothenburg, SE-41296 Gothenburg, Sweden

2. Applied Physics, Division of Material Science, Department of Engineering Science and Mathematics, Luleå University of Technology, SE-97187 Luleå, Sweden

Funder

Vetenskapsrådet

European Cooperation in Science and Technology

Publisher

American Chemical Society (ACS)

Subject

Physical and Theoretical Chemistry

Reference41 articles.

1. Radio Observations of OH in the Interstellar Medium

2. Detection of Interstellar OH in Two External Galaxies

3. Sternberg, A.; Dalgarno, A.; Pei, Y.; Herbst, E.InConditions and Impact of Star Formation;Röllig, M.; Simon, R.; Ossenkopf, V.; Stutzki, J., Eds.EAS Publications Series, 52;European Astronomical Society:Geneva, 2011; pp43–46.

4. A survey of interstellar H I from L-alpha absorption measurements. II

5. The Definitive Abundance of Interstellar Oxygen

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1. Radial molecular property functions of the A2Σ+ state of hydroxyl;Journal of Quantitative Spectroscopy and Radiative Transfer;2021-05

2. Formation of NaCl through radiative association: Computations accounting for non-adiabatic dynamics;The Journal of Chemical Physics;2020-09-21

3. Formation of CO+ by radiative association II;Monthly Notices of the Royal Astronomical Society;2020-01-10

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