On gf values of spectral lines for some diatomic molecules.

Computer Science

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Molecular Data: Stellar Spectra

Scientific paper

The authors have calculated gf values of rotational lines for several molecular band systems in the spectral ranges, commonly used for determining the abundances of C, N, O and isotopic radio 12C/13C in late-type stellar atmospheres. They have compared them with the data from Kurucz' extensive diatomic molecular line lists.

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