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g, the excitation energy differences are 0.06 eV (29) and 0.1636 eV (28), respectively. These energy differences are accounted for in the rate coefficient uncertainties.
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note
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MOLPRO is a package of ab initio programs written by H.-J. Werner and P. J. Knowles, with contributions from J. Almlöf, R. D. Amos, M. J. O. Deegan, S. T. Elbert, C. Hampel, W. Meyer, K. Peterson, R. Pitzer, A. J. Stone, P. R. Taytor, and R. Lindh. Contact molpro-request@tc.bham.ac.uk
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Supported by NASA grants NAG5-4316 and NAG5-4286 and NSF grant ATM-9503224
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Supported by NASA grants NAG5-4316 and NAG5-4286 and NSF grant ATM-9503224.
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