Rotational excitation of molecular ions in interstellar clouds - HCO(+) and HCS(+)

Details Rotational excitation of molecular ions in interstellar clouds - HCO(+) and HCS(+) Rotational excitation of molecular ions in interstellar clouds - HCO(+) and HCS(+)

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210....1m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Sept. 1, 1984, p. 1-11.

Astronomy and Astrophysics

Astrophysics

21

Formyl Ions, Interstellar Gas, Molecular Clouds, Molecular Excitation, Molecular Ions, Molecular Rotation, Collision Rates, Helium, Ionization Cross Sections, Ionization Potentials, Organic Compounds, Sulfur Compounds

Scientific paper

Potential energy surfaces for the HCO+/He and HCS+/He systems have been computed. These surfaces have been used to evaluate collisional cross sections and rate coefficients for the rotational excitation of HCO+ and HCS+ by collision with helium. The astrophysical implications of the results are discussed.

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