Hydrocarbons from shocked carbonaceous dust

Details Hydrocarbons from shocked carbonaceous dust Hydrocarbons from shocked carbonaceous dust

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..280t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 2, p. 280-284.

Astronomy and Astrophysics

Astronomy

6

Cosmic Dust, Erosion, Hydrocarbons, Interstellar Gas, Molecular Ions, Shock Waves, Absorption Spectra, Density (Number/Volume), Signal To Noise Ratios

Scientific paper

Carbonaceous dust is expected to release hydrocarbons upon erosion in
interstellar shocks. When released into predominantly atomic gas, the
subsequent chemistry of these hydrocarbons may lead to detectable
amounts of CH and CH(+). We predict column densities for these molecules
and show how the N(CH+)/N(CH)ratio may constrain the shock parameters.

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