Rotation of the Apsidal Line in the Eclipsing System V1059 Cep

Three light curves of the V1059 Cep eclipsing binary obtained in 2012, 2013, and 2021 were analyzed. We found the rapid apsidal motion in this system at the rate per year. Assuming the equality of observed and theoretical apsidal motion rates we estimated physical characteristics of the components b...

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Veröffentlicht in:	Astronomy reports 2024, Vol.68 (1), p.48-59
Hauptverfasser:	Kozyreva, V. S., Khamrakulov, F. B., Burkhonov, O. A., Bogomazov, A. I., Satovskiy, B. L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Eclipsing binary stars Light curve Observations and Techniques Physical properties Physics Physics and Astronomy
Online-Zugang:	Volltext
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