The chemistry of interstellar CH(+) - The contribution of Bates and Spitzer (1951)

Details The chemistry of interstellar CH(+) - The contribution of Bates and Spitzer (1951) The chemistry of interstellar CH(+) - The contribution of Bates and Spitzer (1951)

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40.1683w&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 12, p. 1683-1693.

Computer Science

4

Carbon Compounds, Hydrogen Compounds, Interstellar Chemistry, Interstellar Matter, Positive Ions, Absorption Spectra, Interstellar Space, Line Spectra, Molecular Ions

Scientific paper

The present evaluation of current understanding of interstellar CH(+) notes that the essential features of this chemistry were identified by Bates and Spitzer in 1951, with more recent work defining those pathways within which these chemical essentials can most efficiently function. Attention is presently given to low temperature gas-phase chemistry in static clouds, interstellar shocks, turbulent interfaces, and photon-dominated regions.

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