The formation of CH/+/ in interstellar clouds

Details The formation of CH/+/ in interstellar clouds The formation of CH/+/ in interstellar clouds

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..633b&link_type=abstract

Astrophysical Journal, vol. 199, Aug. 1, 1975, pt. 1, p. 633-636.

Astronomy and Astrophysics

Astrophysics

54

Hydrocarbons, Interstellar Gas, Ionic Reactions, Molecular Interactions, Nebulae, Abundance, Charge Transfer, Molecular Ions, Photodissociation, Radiative Recombination

Scientific paper

It is suggested that the production of CH(+) in interstellar clouds occurs by a chemical scheme initiated by the radiative association of C(+) and H2. The scheme leads to CH2(+) and CH3(+), which are photodissociated to give CH(+). In contrast to previous formation mechanisms, it is not necessary to suppose that the dissociative recombination of CH(+) is anomalously slow. The same chemical sequence is also able to produce CH in harmony with the measured abundances.

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