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- W1964547152 abstract "Wavelet transform is applied to reanalyze the low amplitude δ Scuti star HD 52788, which exhibits complex light variations with uncertain frequency solutions. We gain an insight into the strong instability of pulsation present in the star. Based on an estimate of the star's physical parameters, its evolutionary status is determined. An attempt of asteroseismic modelling failed to predict the observed dense frequencies. Because of its varying pulsation spectrum, HD 52788 is a distinctive and very interesting object among δ Sct stars for testing current models of stellar evolution and pulsation." @default.
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- W1964547152 date "2004-08-01" @default.
- W1964547152 modified "2023-09-27" @default.
- W1964547152 title "Time-dependent Behaviour of the Low Amplitude δ Scuti Star HD 52788" @default.
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- W1964547152 doi "https://doi.org/10.1088/1009-9271/4/4/335" @default.
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