Dissociative recombination of C2/+/, C2H/+/, C2H2/+/ and C2H3/+/

Details Dissociative recombination of C2/+/, C2H/+/, C2H2/+/ and C2H3/+/ Dissociative recombination of C2/+/, C2H/+/, C2H2/+/ and C2H3/+/

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..749m&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, May 1, 1980, p. 749-751. Research supported by the Natural Sciences and Engineering Re

Astronomy and Astrophysics

Astrophysics

36

Electron-Ion Recombination, Hydrocarbons, Interstellar Chemistry, Molecular Gases, Electron Energy, Gas Dissociation, Polyatomic Molecules, Positive Ions, Reaction Kinetics

Scientific paper

Electron-ion dissociative recombination cross sections have been measured for C2+, C2H+, C2H2+, and C2H3+ over the energy interval from 0.02 to 1 eV using the merged beam technique. Assuming a Maxwellian distribution of the electron velocities, the derived rate coefficient at 100 K for C2+, C2H+, and C2H2+ is found to be 1.0 × 10-6 cm-3 s-1 and for C2H3+, 1.6 × 10-6 cm-3 s-1.

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