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Volumn 131, Issue 22, 2009, Pages

O+OH→O2+H: A key reaction for interstellar chemistry. New theoretical results and comparison with experiment

(10) Lique, F a,g Jorfi, M b Honvault, P b Halvick, P c Lin, S Y d Guo, H d Xie, D Q e Dagdigian, P J f Kos, J g Alexander, M H g

a UNIVERSITÉ DU HAVRE (France)

b UNIVERSITÉ DE FRANCHE COMTÉ (France)

c UNIVERSITÉ DE BORDEAUX (France)

d UNIVERSITY OF NEW MEXICO (United States)

e NANJING UNIVERSITY (China)

f JOHNS HOPKINS UNIVERSITY (United States)

g Bldg 142 (United States)

Author keywords

[No Author keywords available]

Indexed keywords

APPROXIMATE METHODS; COMPARISON WITH EXPERIMENTS; CROSS SECTION; EXPERIMENTAL VALUES; INTERSTELLAR CHEMISTRY; INTERSTELLAR CLOUDS; KEY REACTIONS; LOW COLLISION ENERGY; LOW TEMPERATURES; OH REACTION; QUASICLASSICAL TRAJECTORY CALCULATIONS; THEORETICAL RESULT; WAVE PACKET CALCULATION; YIELD RATES;

APPROXIMATION THEORY; IONIZING RADIATION; MOLECULAR OXYGEN; RATE CONSTANTS;

ATMOSPHERIC TEMPERATURE;

EID: 72449149660 PISSN: 00219606 EISSN: None Source Type: Journal
DOI: 10.1063/1.3274226 Document Type: Article

Times cited : (58)

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