Molecular diagnostics of interstellar shocks

Details Molecular diagnostics of interstellar shocks Molecular diagnostics of interstellar shocks

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..182h&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Feb. 15, 1980, p. 182-188.

Astronomy and Astrophysics

Astrophysics

152

Interstellar Chemistry, Interstellar Gas, Molecular Gases, Shock Wave Propagation, Abundance, Chemical Reactions, Hydrogen Sulfide, Silicon Oxides, Sulfur Oxides

Scientific paper

The chemistry of molecules in shocked regions of the interstellar gas is
considered and calculations are carried out for a region subjected to a
shock at a velocity of 8 km/sec. Substantial enhancements are predicted
in the concentrations of the molecules H2S, SO, and SiO compared to
those anticipated in cold interstellar clouds.

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