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March 3, 2026
TESS light curve and apsidal motion in the eccentric eclipsing binary V871 Aquilae
MW
Marek Wolf
HK
Hana Kučáková
WO
Waldemar Ogłoza
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Key Points
Apsidal motion data highlights the complexity of orbital parameters for V871 Aquilae, enhancing our understanding of binary systems.
Key metrics show significant variations in the light curve, suggesting unique features in the eclipse behavior of the system.
Analysis conducted on the light curve data from TESS to assess the orbital characteristics of the eclipsing binary star.
Findings imply further exploration of eccentric binary systems may provide insights into stellar evolution.
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Wolf et al. (Tue,) studied this question.
synapsesocial.com/papers/69a75a8dc6e9836116a20883
https://doi.org/https://doi.org/10.1016/j.newast.2026.102520
Curva de luz do TESS e movimento apsidal na binária eclipsante excêntrica V871 Aquilae | Synapse