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• W2313018829 abstract "Short-cadence observations of δ Scuti stars in the Kepler field are used to investigate the physical nature of high-amplitude δ Scuti stars (HADS). Although it is often mentioned that HADS are transition objects between classical Cepheids and δ Scuti stars, neither ground-based or space-based observations support this view. It is found that HADS occur randomly within the instability strip. The possibility that HADS may be defined by the presence of combination frequencies is discussed. There is a weak tendency for the number of combination frequencies to increase with increasing amplitude of the parent frequencies. However, even stars with very low amplitudes may have detectable combination frequencies. Very few parent modes have a period ratio appropriate to first-overtone and fundamental radial modes. It appears that a high amplitude, in itself, is not useful as a distinguishing feature of δ Scuti stars." @default.
• W2313018829 created "2016-06-24" @default.
• W2313018829 creator A5083452766 @default.
• W2313018829 date "2016-03-20" @default.
• W2313018829 modified "2023-10-02" @default.
• W2313018829 title "Combination frequencies in high-amplitude δ Scuti stars" @default.
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• W2313018829 doi "https://doi.org/10.1093/mnras/stw671" @default.
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