Abstract
The Franck-Condon (FC) factors (transition probabilities) and r-centroids have been evaluated by the reliable numerical integration procedure for the bands of the b1 Σ+ −x3 Σ− system of astrophysical molecule SO. Also for the bands of f1Δ − a1 Δ and e1 Σ+ − d1 Σ+ systems of astrophysical molecule TiO, the FC factors and r-centroids have been evaluated, using a suitable potential.
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