Frequency Analysis of KIC 1573174: Shedding Light on the Nature of HADS Stars

@article{Lv2022FrequencyAO,
  title={Frequency Analysis of KIC 1573174: Shedding Light on the Nature of HADS Stars},
  author={Chenglong Lv and Ali Esamdin and Javier Pascual-Granado and Tao Yang and Dongxiang Shen},
  journal={The Astrophysical Journal},
  year={2022},
  volume={932}
}
We propose that KIC 1573174 is a quadruple-mode δ Scuti star with pulsation amplitudes between those of the high-amplitude Delta Scuti star group and average low-amplitude pulsators. The radial modes detected in this star provide a unique opportunity to exploit asteroseismic techniques up to their limits. Detailed frequency analysis is given for the light curve from the Kepler mission. The variation of the light curve is dominated by the strongest mode with a frequency of F0 = 7.3975 day−1, as… 

Asteroseismology of a Double-mode High-amplitude δ Scuti Star TIC 448892817

We propose that TIC 448892817 is a double-mode high-amplitude δ Scuti star. The radial modes detected in this star provide a unique opportunity to exploit asteroseismic techniques up to their limits.

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