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• W1726584611 abstract "We present a period analysis of the light curve and its Fourier parameters of the bright Cepheid V1154 Cyg (P=4.925454 days) based on the observations by the Kepler space telescope. Fourier parameters R21, R31 clearly indicate variations with a period of 158.2 ± 1 days (more than 5σ peak in the power spectrum) with a very small amplitude (0.265-0.275 for R21, 0.065-0.071 for R31) making impossible to detect it with ground- based observations. Finally we discuss that this effect is similar to the Blazhko effect in RR Lyrae stars." @default.
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• W1726584611 date "2015-01-01" @default.
• W1726584611 modified "2023-09-23" @default.
• W1726584611 title "Long term light curve variations of theKeplerCepheid V 1154 Cyg" @default.
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• W1726584611 doi "https://doi.org/10.1051/epjconf/201510106036" @default.
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