Connections between the cycle-to-cycle light curve and O-C variations of the Blazhko RR Lyrae stars
J\'ozsef M. Benk\H{o}

TL;DR
This study investigates the link between cycle-to-cycle light curve variations and O-C diagram irregularities in Blazhko RR Lyrae stars, revealing a strong correlation with the Blazhko effect amplitude using Kepler data.
Contribution
It extends analysis of C2C light curve variations to Blazhko stars, demonstrating their significant role in O-C irregularities and their correlation with the Blazhko effect.
Findings
C2C variations are present in 74% of Blazhko stars' O-C diagrams.
The strength of C2C variations is larger in Blazhko stars than in non-Blazhko stars.
A strong positive correlation exists between C2C variation strength and Blazhko amplitude.
Abstract
Recent studies have shown that the irregular O-C variations observed in many non-Blazhko RR Lyrae stars may result from random, cycle-to-cycle (C2C) variations in their light curves. However, centuries-long data series reveal that the O-C diagrams of Blazhko stars exhibit particularly large-amplitude, irregular variations. In this Letter, we extend the previous investigation of non-Blazhko stars to Kepler Blazhko stars to explore the role of C2C variations in the O-C diagrams. We derived the O-C diagrams from Kepler space telescope light curves using a precise template-fitting method. Based on their Fourier analyses, we also constructed residual O-C diagrams that were pre-whitened for frequencies associated with the Blazhko effect. We then fitted the same statistical models to both types of O-Cs that we had previously applied to non-Blazhko stars. The optimal statistical model includes…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Scientific Research and Discoveries
