HD 519401 A Probable New Heartbeat Star System

HD-51940 is a system with periodic variations in its light curve that resemble those of heartbeat stars(HBS). The system's host shows periodic flux changes. The period is approximately 1.87 days, with a transit depth of 0.15%. However, further research needs more information to study this system. It was initially classified as a possible host of a transiting planet. The number of potential hosts in the system is a mystery. Could HD-51940 be a heartbeat star? To find the answer, we first compared the characteristics of HD-51940 with other defined HBS. We used the Kumar model to fit the light curve and best period of HD-51940, and last, we computed the Fourier transform of the light curve to seek evidence for tidally induced oscillations that would be diagnostic of a heartbeat star. In our conclusion, the surge of flux on the light curve became apparent after we processed and fit the data. In addition, the periodic signal was found. Hence, we determined that HD-51940 is an HBS.

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Publication Details

Journal
Theoretical and Natural Science
Published
2025-05-06
DOI
https://doi.org/10.54254/2753-8818/2025.22668
Primary Topic
History and Developments in Astronomy
Type
article
Field-Weighted Citation Impact
0.00

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article

HD 519401 A Probable New Heartbeat Star System

Hang Yu, Tian Qiu, Changxuan Li, Yu‐Tai Tao et al.
Theoretical and Natural Science
History and Developments in Astronomy
article

HD 519401 A Probable New Heartbeat Star System

Hang Yu, Tian Qiu, Changxuan Li, Yu‐Tai Tao, Yushu Liub
article en

Abstract

HD-51940 is a system with periodic variations in its light curve that resemble those of heartbeat stars(HBS). The system's host shows periodic flux changes. The period is approximately 1.87 days, with a transit depth of 0.15%. However, further research needs more information to study this system. It was initially classified as a possible host of a transiting planet. The number of potential hosts in the system is a mystery. Could HD-51940 be a heartbeat star? To find the answer, we first compared the characteristics of HD-51940 with other defined HBS. We used the Kumar model to fit the light curve and best period of HD-51940, and last, we computed the Fourier transform of the light curve to seek evidence for tidally induced oscillations that would be diagnostic of a heartbeat star. In our conclusion, the surge of flux on the light curve became apparent after we processed and fit the data. In addition, the periodic signal was found. Hence, we determined that HD-51940 is an HBS.

Theoretical and Natural ScienceVol. 107(1)
Beijing Haidian Hospital (CN), Renmin University of China (CN)
Princeton University
Openalex Percentile: Top 93%
History and Developments in Astronomy
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HD 519401 A Probable New Heartbeat Star System — Hang Yu, Tian Qiu, et al. · Theoretical and Natural Science (2025) | TGRS Research Map | TGRS