Molecular abundances in dense interstellar clouds (Lee+ 1996)

Details Molecular abundances in dense interstellar clouds (Lee+ 1996) Molecular abundances in dense interstellar clouds (Lee+ 1996)

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41190111l&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/119/111. Originally published in: 1996A&AS..119..111L

Physics

Interstellar Medium, Abundances

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 - 1,000; 10,000; and 100,000cm-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.
(28 data files).

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