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Paper: Frequency Regularities in δ Scuti Stars
Volume: 479, Progress in Physics of the Sun and Stars
Page: 91
Authors: Paparó, M.; Benkő, J. M.
Abstract: Space missions have produced an incredibly large database on pulsating stars. The light curves via the frequency content contain a detailed description of each star. The critical point is the identification of modes, especially in the non-asymptotic regime. The best derived parameters from the frequency content of a pulsating star light curve are the frequency differences and ratios. This presentation focuses on the potential of period ratios in mode identification.
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