Fractional abundances of molecules in dense interstellar clouds: A compendium of recent model results.

Details Fractional abundances of molecules in dense interstellar clouds: A compendium of recent model results. Fractional abundances of molecules in dense interstellar clouds: A compendium of recent model results.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..119..111l&link_type=abstract

Astronomy and Astrophysics Supplement, v.119, p.111-114

Astronomy and Astrophysics

Astrophysics

167

Ism: Clouds, Ism: Abundances, Ism: Molecules, Molecular Processes

Scientific paper

In this paper we present calculated fractional abundances in dense interstellar clouds for selected atomic and molecular species using three different homogeneous, pseudo-time-dependent models discussed by Bettens, Lee, & Herbst (1995): the new standard model, the new neutral-neutral model, and model 4. We have run each model with 3 different hydrogen densities - 10^3^, 10^4^, and 10^5^cm^-3^ - and two temperatures - 10K and 50K. "Low metal" elemental abundances have been used for all three models; the new standard model has also been run with "high metal" abundances.

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