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Rate constant for OH([sup 2]Π)+O([sup 3]P)→H([sup 2]S)+O[sub 2]([sup 3]Σ[sub g][sup −]) reaction on an improved ab initio potential energy surface and implications for the interstellar oxygen problem

✍ Scribed by Xu, Chuanxiu; Xie, Daiqian; Honvault, Pascal; Lin, Shi Ying; Guo, Hua


Book ID
120655211
Publisher
American Institute of Physics
Year
2007
Tongue
English
Weight
462 KB
Volume
127
Category
Article
ISSN
0021-9606

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