Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248l..19c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. L19-L21.
Astronomy and Astrophysics
Astrophysics
31
Formyl Ions, Gas Dissociation, Hydrogen Ions, Interstellar Chemistry, Molecular Ions, Recombination Coefficient, Cosmochemistry, Ion Recombination, Positive Ions
Scientific paper
A flowing-afterglow apparatus operating at 300 K has been used to measure the dissociative recombination rate coefficients of H3(+), with low vibrational excitation, as well as HCO(+). While the results obtained are in agreement with those of Amano (1990), they contradict the study of Adams and Smith (1988). It is concluded that there is no measurable vibration dependence in the dissociative recombination-rate coefficient, at least in the cases of several low-lying vibrational states.
Canosa André
Gomet J. C.
Mitchell J. B. A.
Rebrion C.
Rowe Bertrand R.
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