作者: K. M. Hickson , S. J. Klippenstein , J. C. Loison , W. D. Geppert , A. Bergeat
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摘要: Predictions of astrochemical models depend strongly on the reaction rate coefficients used in simulations. We reviewed a number key reactions for chemistry nitrogen-bearing species dense interstellar medium and proposed new those reactions. The details reviews are given form datasheet associated with each reaction. recommended an uncertainty temperature range validity will be included KIDA (http://kida.obs.u-bordeaux1.fr).