On the connection between almost periodic functions and Blazhko light curves

Abstract

In this paper it is shown that the mathematical form which most precisely describes the Blazhko RR Lyrae light curves is connected to almost periodic functions and not to the mathematics of modulation. That is, the Blazhko effect is more than a simple external modulation of the pulsation signal. The mathematical framework of almost periodic functions predicts a new observable effect: a shift of the Fourier harmonics of the main pulsation frequency from the exact harmonic position. This phenomenon is called as harmonic detuning effect (HDE).The published deviations of the harmonics of V445 Lyr are explained with this effect. HDE is also found for V2178 Cyg, another Blazhko star observed by the Kepler space telescope. HDE is detectable only if the phase variation part of the Blazhko effect is of large amplitude and non-periodic enough, additionally, the time span of the observed light curve is sufficiently long for obtaining precise frequencies. These three conditions restrict the number of stars showing detectable HDE and explain why this effect has not been discovered up to now.

arXiv comment8 pages, 2 figures, accepted for publication in MNRAS

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Cited by in corpus (6)

• Blazhko effect in the Galactic bulge fundamental mode RR Lyrae stars II: Modulation shapes, amplitudes and periods
• Revisiting the Kepler non-Blazhko RR Lyrae sample: Cycle-to-cyle variations and additional modes
• Periodic Variable Stars Modulated by Time-Varying Parameters
• Big Signals, Small Signals, Systematics
• Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars
• The spectral Petersen diagram as a new tool to map pulsation modes in variable stars