The formation of molecules in diffuse interstellar clouds

Details The formation of molecules in diffuse interstellar clouds The formation of molecules in diffuse interstellar clouds

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...212...71m&link_type=abstract

Astrophysical Journal, Part 1, vol. 212, Feb. 15, 1977, p. 71-78. Research supported by the National Research Council of Canada

Astronomy and Astrophysics

Astrophysics

19

Hydrocarbons, Interstellar Matter, Molecular Spectra, Abundance, Astrophysics, Gas Density, Photoionization

Scientific paper

A chemical system involving carbon and hydrogen is used to obtain steady-state abundances of a number of molecules over a wide range of densities. The calculated CH abundance agrees well with the astronomical observations. For reasonable values of the rate coefficients, the present system of reactions cannot explain, simultaneously, the measured abundances of CH and CH(+). An abundance of C2H comparable to the abundance of CH is predicted for diffuse clouds.

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