Dissociative Recombination of Rotationally Cold OH+ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds

Observations of OH ^+ are used to infer the interstellar cosmic ray ionization rate in diffuse atomic clouds, thereby constraining the propagation of cosmic rays through and the shielding by interstellar clouds, as well as the low energy cosmic ray spectrum. In regions where the H _2 -to-H number de...

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Автори:	Ábel Kálosi, Lisa Gamer, Manfred Grieser, Robert von Hahn, Leonard W. Isberner, Julia I. Jäger, Holger Kreckel, David A. Neufeld, Daniel Paul, Daniel W. Savin, Stefan Schippers, Viviane C. Schmidt, Andreas Wolf, Mark G. Wolfire, Oldřich Novotný
Формат:	Artigo
Мова:	Inglês
Опубліковано:	IOP Publishing 2023-01-01
Серія:	The Astrophysical Journal Letters
Предмети:	Diffuse interstellar clouds Diffuse molecular clouds Laboratory astrophysics Electron recombination reactions Reaction rates Astrochemistry
Онлайн доступ:	https://doi.org/10.3847/2041-8213/acf71d
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Dissociative Recombination of Rotationally Cold OH+ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds

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