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Insights into H(2) formation in space from ab initio molecular dynamics
Hydrogen formation is a key process for the physics and the chemistry of interstellar clouds. Molecular hydrogen is believed to form on the carbonaceous surface of dust grains, and several mechanisms have been invoked to explain its abundance in different regions of space, from cold interstellar clo...
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| Autori principali: | , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
National Academy of Sciences
2013
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3637713/ https://ncbi.nlm.nih.gov/pubmed/23572584 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1301433110 |
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