Silicate-mediated interstellar water formation: A theoretical study.
ISM: atoms
ISM: molecules
astrochemistry
molecular processes
Journal
Monthly notices of the Royal Astronomical Society
ISSN: 0035-8711
Titre abrégé: Mon Not R Astron Soc
Pays: England
ID NLM: 100954591
Informations de publication
Date de publication:
14 May 2019
14 May 2019
Historique:
entrez:
4
6
2019
pubmed:
4
6
2019
medline:
4
6
2019
Statut:
ppublish
Résumé
Water is one of the most abundant molecules in the form of solid ice phase in the different regions of the interstellar medium (ISM). This large abundance cannot be properly explained by using only traditional low temperature gas-phase reactions. Thus, surface chemical reactions are believed to be major synthetic channels for the formation of interstellar water ice. Among the different proposals, hydrogenation of atomic O (
Identifiants
pubmed: 31156274
doi: 10.1093/mnras/sty3024
pmc: PMC6544534
mid: EMS82852
doi:
Types de publication
Journal Article
Langues
eng
Pagination
5389-5400Subventions
Organisme : European Research Council
ID : 610256
Pays : International
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