Methanol Formation via the Radical–Radical Reaction of OH and CH3 Radicals Undergoing Transient Diffusion on Ice at 10 to 60 K

Methanol (CH _3 OH) is thought to form on interstellar ice dust via successive hydrogenation reactions. The reaction between CH _3 and OH radicals could also conceivably generate methanol at temperatures above approximately 20 K, at which temperature hydrogen atoms will not adhere to the ice surface...

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Hlavní autoři:	Arisa Iguchi, Hiroshi Hidaka, Atsuki Ishibashi, Masashi Tsuge, Yasuhiro Oba, Naoki Watanabe
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	Dense interstellar clouds Interstellar dust processes Astrochemistry
On-line přístup:	https://doi.org/10.3847/1538-4357/ae381b
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