Laboratory studies of some ion-atom reactions related to interstellar molecular synthesis

Details Laboratory studies of some ion-atom reactions related to interstellar molecular synthesis Laboratory studies of some ion-atom reactions related to interstellar molecular synthesis

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..492v&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Mar. 1, 1980, p. 492-497. Research supported by the U.S. Defense Nuclear Agency and Oe

Physics

29

Interstellar Chemistry, Interstellar Matter, Ion Atom Interactions, Molecular Physics, Reaction Kinetics, Electron-Ion Recombination, Molecular Ions, Neutral Atoms, Positive Ions

Scientific paper

The rate coefficients and product ions have been determined for reactions involving C(+), CH(+), CH2(+), CH3(+), CH5(+), C2(+), C2H(+), C2H2(+), D(+), OH(+), and H2O(+) ions with N and O atoms and NO molecules at 300 K. The values obtained for the rate coefficients are generally substantial fractions of the collision-limiting values, indicating that ion-atom reactions can be important steps in the synthesis of some of the molecules observed in interstellar clouds, in accordance with previous models.

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