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Low temperature rates for key steps of interstellar gas-phase water formation
The gas-phase formation of water molecules in the diffuse interstellar medium (ISM) proceeds mainly via a series of reactions involving the molecular ions OH(+), H(2)O(+), and H(3)O(+) and molecular hydrogen. These reactions form the backbone for the chemistry leading to the formation of several com...
| Autores principales: | , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
American Association for the Advancement of Science
2018
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6014714/ https://www.ncbi.nlm.nih.gov/pubmed/29942857 http://dx.doi.org/10.1126/sciadv.aar3417 |