The dissociative recombination of CH/plus/ ions

Details The dissociative recombination of CH/plus/ ions The dissociative recombination of CH/plus/ ions

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...214l.101g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 214, June 1, 1977, p. L101-L103. NATO-supported research.

Astronomy and Astrophysics

Astrophysics

19

Electron Orbitals, Interstellar Chemistry, Reaction Kinetics, Recombination Reactions, Electron Recombination, Interstellar Matter, Ion Recombination, Metastable State

Scientific paper

Calculations of excited states of CH, including diffuse orbitals in the atomic-function basis set, suggest a rate coefficient for dissociative recombination of CH (plus) ions that is much smaller than 10 to the -7th power cu cm/s. The reduced rate coefficient may lead to a better agreement with the observed abundance of CH(plus) in diffuse interstellar clouds.

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