Dense cloud chemistry. III - The detailed chemical network and the effects of parameter variation

Details Dense cloud chemistry. III - The detailed chemical network and the effects of parameter variation Dense cloud chemistry. III - The detailed chemical network and the effects of parameter variation

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..87..435m&link_type=abstract

Astrophysics and Space Science, vol. 87, no. 1-2, Oct. 1982, p. 435-453.

Astronomy and Astrophysics

Astrophysics

4

Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Abundance, Hydrogen Sulfide, Sulfur Compounds, Tables (Data)

Scientific paper

The detailed reaction network used in Paper I of this series is presented and the sensitivity of the calculated abundances of sulphur-bearing species to various parameters including reaction efficiency and elemental depletions is discussed. It is shown that while ion-grain reactions can provide appreciable abundances of many S-bearing species, they do not contribute significantly to the abundance of O-bearing molecules. Observations of HDS in interstellar clouds could provide important information on the formation of H2S.

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