KIC 10855535: An elegant Delta Scuti pulsator with Amplitude and Phase Modulation
Lixian Shen, Ali Esamdin, Chenglong Lv, Haozhi Wang, Taozhi Yang,, Rivkat Karimov, Shuhrat A. Ehgamberdiev, Hubiao Niu, Jinzhong Liu

TL;DR
This study analyzes KIC 10855535, a Delta Scuti star, revealing its binary nature, pulsation characteristics, and signs of stellar evolution through amplitude and phase modulation over four years of Kepler data.
Contribution
The paper provides a detailed analysis of pulsation modes, binary orbit, and evolutionary indicators in KIC 10855535, highlighting its slow rotation and amplitude/phase modulation in a Delta Scuti star.
Findings
Detection of fundamental and low-frequency pulsation modes.
Confirmation of binarity through phase modulation and orbital parameters.
Observation of amplitude growth suggesting stellar structural changes.
Abstract
We investigated the pulsating behavior of KIC 10855535 using Kepler 4-year long cadence data. Two independent frequencies were detected: a pulsation frequency F0 = 17.733260(5)d-1 and a low frequency f8=0.412643(8)d-1 We identify F0 as the fundamental frequency, at which a equidistant quintuplet is centered, suggesting that the star orbits in a binary system. The fitted orbital parameters align well with those reported in previous literature. Long-term phase modulation caused by binarity has been confirmed by considering TESS light curve. Through adjusting light time via removing the light time effect, we measured a linear change in period of order , a value that could be indicative of stellar evolution. The star also exhibits a gradual and stable amplitude growth, thereby raising the possibility of structural changes during its evolution. We…
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