Chemical modelling of dark clouds in the LMC and SMC

Details Chemical modelling of dark clouds in the LMC and SMC Chemical modelling of dark clouds in the LMC and SMC

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242...92m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 1, 1990, p. 92-97. Research supported by SERC

Astronomy and Astrophysics

Astronomy

19

Astronomical Models, Dark Matter, Interstellar Chemistry, Magellanic Clouds, Carbon Monoxide, Chemical Composition, Hydrocarbons, Molecular Ions, Time Dependence

Scientific paper

Pseudotime-dependent model calculations of the chemistry of dark clouds in the LMC and SMC have been undertaken. Molecular abundances have been determined for a variety of species both at 'early time' and at steady state. Many of the calculated molecular abundances depend, in a complex manner, on the differing elemental abundances of C, O, and N in the LMC and SMC. One excetption is the abundance of CO which depends linearly on the elemental carbon abundance in regions where the O/C abundance ratio exceeds unity.

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