Depletion of ethanol by reaction with OH radicals at typical temperatures of the dense molecular clouds of the interstellar medium (21-107 K) - Archive ouverte HAL Accéder directement au contenu
Poster De Conférence Année : 2017
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hal-01681447 , version 1 (11-01-2018)

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  • HAL Id : hal-01681447 , version 1

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Sergio Blázquez, Antonio Ocaña, Maria Antinolo, Bernabé Ballesteros, André Canosa, et al.. Depletion of ethanol by reaction with OH radicals at typical temperatures of the dense molecular clouds of the interstellar medium (21-107 K). Workshop of the WG1 of the COST CM1401 Our Astrochemical history program: "Gas phase cold chemistry of COMs: a challenge for experiments, theory, and astrophysical modelling", Dec 2017, Ciudad Real, Spain. ⟨hal-01681447⟩
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