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Gas Phase Kinetics of the OH+CH(3)CH(2)OH Reaction at Temperatures of the Interstellar Medium (T = 21-107 K)
Ethanol, CH(3)CH(2)OH, has been unveiled in the interstellar medium (ISM) by radioastronomy and it is thought to be released into the gas phase after the warm-up phase of the grain surface, where it is formed. Once in the gas phase, it can be destroyed by different reactions with atomic and radical...
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| 出版年: | Phys Chem Chem Phys |
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| 主要な著者: | , , , , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
2018
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| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5975950/ https://ncbi.nlm.nih.gov/pubmed/29417104 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1039/c7cp07868d |
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