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Silicate-mediated interstellar water formation: A theoretical study
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 m...
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| Publicado no: | Mon Not R Astron Soc |
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| Main Authors: | , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2019
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6544534/ https://ncbi.nlm.nih.gov/pubmed/31156274 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/sty3024 |
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