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- W2986566057 abstract "Abstract CCD observations of V367 Cam, a high-amplitude δ Scuti star, were carried out in both V and R band on October 22 and 23 and November 4, 2016. By using the new observed maximum times and the previously reported epochs, a new ephemeris is obtained. Fourier analysis of the light curves yields the main frequency f1 = 8.2242 d −1 and its second harmonic as 2f1 = 16.4062 d −1. The pulsation constant specifying the oscillation characteristics of pulsating stars is calculated from physical parameters of V367 Cam. We obtained Q = 0.03814 ± 0.00409, which demonstrates this star pulsates in single radial fundamental mode. With the derived physical parameters, the evolution status of V367 Cam is determined and also it is shown on H-R diagram against other δ Scuti stars. Furthermore, we made a count of mono-periodic HADS, which are expected to be decreasing in number and turned to be multiperiodic in the advent of high precision photometry and extended data." @default.
- W2986566057 created "2019-11-22" @default.
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- W2986566057 date "2020-05-01" @default.
- W2986566057 modified "2023-09-24" @default.
- W2986566057 title "An observational study of the high-amplitude δ Scuti star V367 Cam" @default.
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- W2986566057 doi "https://doi.org/10.1016/j.newast.2019.101338" @default.
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