Numerical studies of collapsing interstellar clouds

Details Numerical studies of collapsing interstellar clouds Numerical studies of collapsing interstellar clouds

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nasa.reptq....b&link_type=abstract

Final Technical Report National Aeronautics and Space Administration. Ames Research Center, Moffett Field, CA.

Mathematics

Abundance, Interstellar Matter, Mathematical Models, Molecular Clouds, Radiative Transfer, Chemical Properties, Line Spectra, Prediction Analysis Techniques, Thermodynamic Properties, Time Dependence

Scientific paper

Numerical simulation of the structure and evolution of interstellar clouds was initiated. Steps were taken toward an integrated treatment of the dynamical, thermal, and chemical processes entering model calculations. A detailed study was made of radiative transfer in molecular lines to allow model predictions to be tested against empirical data. The calculations have successfully reproduced and explained several observed cloud properties, including abundances of complex molecular species and the apparent depletion of CO in dense cores.

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