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Rotational line strengths, computed from eigenvectors of Hund's case (a)matrix representations of the upper and lower Hamiltonians using Wigner-Witmerbasis functions, show a larger than expected influence from the well knownperturbation in the (5,4) band. Comparisons with National Solar Observatoryexperimental Fourier transform spectroscopy data reveal nice agreement ofmeasured and predicted spectra.  Keywords: Diatomic spectroscopy, rotational line strengths, H\"onl-Londonfactors, cyanide spectra violet band perturbations

Rotational line strengths for the CN $B \, ^2\Sigma^+ - X \, ^2\Sigma^+$ (5,4) band