VIBRATION-ROTATIONAL INTENSITIES FOR DIATOMIC MOLECULES OF ASTROPHYSICAL INTEREST: THE ISOVALENT MOLECULES CO, CS, SiO AND SiS

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1987

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Ohio State University

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Vibration-rotational dipole moment matrix elements and Einstein A coefficients have been calculated for a group of isovalent molecules of astrophysical interest. The wavefunctions used were obtained by a direct numerical integration of the radial Schrodinger equation with an RKR potential-energy function. The dipole-moment functions were represented by Pade approximants which have the correct theoretical long-range dependence on the internuclear separation. The coefficients in these expressions were obtained for CO, CS and SiO from experimental intensity data and/or ab initio calculations. For SiS for which only the permanent dipole moment is known, we estimated the intensities from the systematic trends found for the other three isovalent molecules.

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Author Institution: Department of Physics and Astronomy, University of Alabama; Department of Physics and Astronomy, NASA Ames Research Center

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