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Gas Phase Kinetics of the OH+CH(3)CH(2)OH Reaction at Temperatures of the Interstellar Medium (T = 21-107 K)

Ethanol, CH(3)CH(2)OH, has been unveiled in the interstellar medium (ISM) by radioastronomy and it is thought to be released into the gas phase after the warm-up phase of the grain surface, where it is formed. Once in the gas phase, it can be destroyed by different reactions with atomic and radical...

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Detalhes bibliográficos
Publicado no:Phys Chem Chem Phys
Main Authors: Ocaña, A. J., Blázquez, S., Ballesteros, B., Canosa, A., Antiñolo, M., Albaladejo, J., Jiménez, E.
Formato: Artigo
Idioma:Inglês
Publicado em: 2018
Assuntos:
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC5975950/
https://ncbi.nlm.nih.gov/pubmed/29417104
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1039/c7cp07868d
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