Recent Advances in Calculating Molecular Collision Rates

Details Recent Advances in Calculating Molecular Collision Rates Recent Advances in Calculating Molecular Collision Rates

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..855..245w&link_type=abstract

ASTROCHEMISTRY: From Laboratory Studies to Astronomical Observations. AIP Conference Proceedings, Volume 855, pp. 245-252 (2006

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Atomic, Molecular, And Chemical, And Grain Processes, Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds, Rotational And Vibrational Energy Transfer, Absolute And Relative Line And Band Intensities

Scientific paper

Interstellar clouds are mainly composed of hydrogen molecules whose molecular spectra are difficult to record. Major other components are polar molecules, whose rotational and ro-vibrational spectra are readily observed. Inelastic collisions of molecules with H2 and electrons are important processes to understand the formation and intensities of molecular spectral lines. We have calculated the interaction energy and various inelastic cross-sections and rates, for two important constituents of the interstellar media, H2O and HC3N.

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