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OH+IN ASTROPHYSICAL MEDIA: STATE-TO-STATE FORMATION RATES, EINSTEIN COEFFICIENTS AND INELASTIC COLLISION RATES WITH He
The rate constants required to model the OH^+ observations in different regions of the interstellar medium have been determined using state of the art quantum methods. First, state-to-state rate constants for the H_2(v=0,J=0,1)+ O^+(^4S) → H + OH^+(X ^3Σ^-, v', N) reaction have been obtained using a quantum wave packet method. The calculations have been compared with time-independent results to asses the accuracy of reaction probabilities at collision energies of about 1 meV. The good agreementdoi:10.1088/0004-637x/794/1/33 fatcat:3ea3ubavifeu3a6lmqivh7odqi