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...

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Detalles Bibliográficos
Autores principales: Kumar, Sunil S., Grussie, Florian, Suleimanov, Yury V., Guo, Hua, Kreckel, Holger
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2018
Materias:
Research Articles
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

Internet

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

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