J. N. Bardsley, B. R. Junker
Abstract
Preliminary calculations of excited states of CH suggest a rate of order 1O- cm3 -1 for the dissociative recombination process e + CH+ (X 1 +) C('D) + H. Such a large rate would necessitate considerable revision of some recent models of interstellar douds. Subject headings:interstellar matter - molecules, interstellar
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Preliminary calculations of excited states of CH suggest a rate of order 1O- cm3 -1 for the dissociative recombination process e + CH+ (X 1 +) C('D) + H. Such a large rate would necessitate considerable revision of some recent models of interstellar douds. Subject headings:interstellar matter - molecules, interstellar
Key concepts: Dissociative recombination, Physics, Ion, Excited state, Astrophysics, Recombination, Molecule, Atomic physics