Franck-Condon factors, r-centroids and oscillator strength of BaO (A1σ−X1σ)

Wentink, Tunis; Spindler, Robert J.

doi:10.1016/0022-4073(72)90028-3

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Cited by 22 publications

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“…We used the following references to identify the strong TiO features:. Gatterer, Junkes, Salpeter and Rosen (1957), Phillips (1969Phillips ( , 1971, Phillips and Davis (1971), Wentink and Spindler (1972). The MgH depressions (Moore et al 1966) are very strong on our spectra, as can be seen in Figures 1-6.…”

Section: Observationssupporting

confidence: 62%

Scanner observations of selected cool stars

Fay

Stein

Warren

1974

PASP

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Photoelectric spectral scans at 30-1 resolution of 9 dwarfs, 10 giants and 6 supergiants with spectral types GO to M5 are presented. All stars were observed every 4 j from X3300 to 47000. Absorption features observed at this resolution coincide with.' strong atomic lines of Fe I,II, Ca I,II, MgI, and Na I; vibrational bands of the electronic transitions of TiO, MgH, CaH, SiH, AlH, CN, CH, C 2 , OH, and NH. The dependence of the 4 3 7 40 Fe I blend and the X3440 depression on temperature is discussed.

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Section: Observationssupporting

confidence: 62%

Scanner observations of selected cool stars

Fay

Stein

Warren

1974

PASP

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Resonant and Near‐Resonant Rayleigh and Raman Scattering for a Diatomic Molecule

Berg¹,

Robinson

1977

Israel Journal of Chemistry

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Using the results of a unified theory of scattering in the time‐independent (narrow exciting line) limit, excitation profiles for Rayleigh and Raman cross sections have been calculated for an actual diatomic molecule from over 8000 cm−1 off resonance into the resonance region. Three interference effects, a “vibrational level interference”, an “on‐resonance Franck—Cordon interference”, and “off‐resonance interference,” are discussed.

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One hundred and fifty-three diatomic molecules, molecular ions, and radicals of astrophysical interest

Singh

Chaturvedi

1987

Astrophys Space Sci

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Franck-Condon factors, r-centroids and oscillator strength of BaO (A1σ−X1σ)

Cited by 22 publications

References 8 publications

Scanner observations of selected cool stars

Scanner observations of selected cool stars

Resonant and Near‐Resonant Rayleigh and Raman Scattering for a Diatomic Molecule

One hundred and fifty-three diatomic molecules, molecular ions, and radicals of astrophysical interest

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