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- W3098867247 abstract "Time-series photometric observations were made for the High Amplitude $delta$ Scuti star CW Ser between 2011 and 2012 at the Xinglong Station of National Astronomical Observatories of China. After the frequency analysis of the light curves, we confirmed the fundamental frequency of $f = 5.28677 cd^{-1}$, together with 8 harmonics of the fundamental frequency, 7 of which are newly detected. No additional frequencies were detected. The O-C diagram, produced with the 21 newly determined times of maximum light combined with those provided in the literature, helps to obtain a new ephemeris formula of the times of maximum light with the pulsation period of $0.189150355 pm 0.000000003 days$." @default.
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- W3098867247 date "2013-09-27" @default.
- W3098867247 modified "2023-10-16" @default.
- W3098867247 title "Pulsation analysis of the high amplitude δ Scuti star CW Serpentis" @default.
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- W3098867247 doi "https://doi.org/10.1088/1674-4527/13/10/004" @default.
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