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KIC 10855535: An Elegant δ Scuti Pulsator with Amplitude and Phase Modulation

Lixian ShenXinjiang Astronomical Observatory,Chinese Academy of Sciences, Urumqi,Xinjiang 830011,People's Republic of ChinaAli EsamdinXinjiang Astronomical Observatory,Chinese Academy of Sciences, Urumqi,Xinjiang 830011,People's Republic of ChinaChenglong LvXinjiang Astronomical Observatory,Chinese Academy of Sciences, Urumqi,Xinjiang 830011,People's Republic of ChinaHaozhi WangXinjiang Astronomical Observatory,Chinese Academy of Sciences, Urumqi,Xinjiang 830011,People's Republic of ChinaTao-Zhi YangMinistry of Education Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, School of Physics, Xi'an Jiaotong University, Xi'an 710049, People's Republic of ChinaR. KarimovUlugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomicheskaya 33, Tashkent, 100052, UzbekistanSh. A. EhgamberdievUlugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomicheskaya 33, Tashkent, 100052, UzbekistanHubiao NiuXinjiang Astronomical Observatory,Chinese Academy of Sciences, Urumqi,Xinjiang 830011,People's Republic of ChinaJinzhong LiuSchool of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
The Astrophysical Journaljournal2024en
ABI

Аннотация

Abstract We investigated the pulsating behavior of KIC 10855535 using Kepler 4 yr long-cadence data. Two independent frequencies were detected: a pulsation frequency F0 = 17.733260(5) day −1 and a low frequency f 8 = 0.412643(8) day −1 . We identify F0 as the fundamental frequency, at which an 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 the light curve from the Transiting Exoplanet Survey Satellite. By removing the light-time effect, we measured a linear change in period of order <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mover accent="true"> <mml:mrow> <mml:mi>P</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>̇</mml:mo> </mml:mrow> </mml:mover> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:mi>P</mml:mi> <mml:mo>≃</mml:mo> <mml:mn>1.44</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mrow> <mml:mn>10</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>7</mml:mn> </mml:mrow> </mml:msup> <mml:mspace width="0.25em"/> <mml:msup> <mml:mrow> <mml:mi>yr</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:math> , 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 attributed f 8 and its two harmonics to rotation and surface spots, with further analysis suggesting characteristics evolving over time. Based on this hypothesis, KIC 10855535 may rotate slowly for its type, with a speed of 37(2) km s −1 . Overall, KIC 10855535 presents an exceptionally clean spectrum and a relatively slow rotation as a δ Sct pulsator, exhibiting a single pulsation mode that undergoes both amplitude and phase modulation.

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