Collisional excitation of interstellar molecule due to H2. II - Excited rotational-vibrational states of SiO

Details Collisional excitation of interstellar molecule due to H2. II - Excited rotational-vibrational states of SiO Collisional excitation of interstellar molecule due to H2. II - Excited rotational-vibrational states of SiO

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78..463m&link_type=abstract

Astrophysics and Space Science, vol. 78, no. 2, Aug. 1981, p. 463-465. Research supported by the University Grants Commission.

Astronomy and Astrophysics

Astrophysics

3

Hydrogen, Interstellar Matter, Molecular Collisions, Molecular Excitation, Molecular Oscillations, Silicon Oxides, Rates (Per Time), Tables (Data)

Scientific paper

Collision induced vibrational rates of SiO due to H2 are computed using
the normalized per- turbative, semiclassical approach as described in
Paper I (Mehrotra, 1980). The rates are very small as compared to the
rates for rotational excitation and are more sensitive to temperature

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