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arXiv · 1309.4888

Kepler RR Lyrae stars: beyond period doubling

L. Molnár·J. M. Benkő·R. Szabó·Z. Kolláth
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Abstract

We examined the complete short cadence sample of Kepler RR Lyrae stars to further investigate the recently discovered dynamical effects such as period doubling and additional modes. Here we present the findings on four stars. V450 Lyr may be a non-classical double-mode RR Lyrae star pulsating in the fundamental mode and the second overtone. In three cases we observe the interaction of three different modes. Since the period ratios are close to resonant values, we observe quasi-repetiting patterns in the pulsation cycles in the stars. These findings support the mode-resonance explanations of the Blazhko effect.

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L. Molnár, J. M. Benkő, R. Szabó, Z. Kolláth. 2013-09-19. Kepler RR Lyrae stars: beyond period doubling. https://doi.org/10.1017/s1743921313015044

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