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首页> 外文期刊>Astrophysics and space science >Light curve solutions of the eclipsing eccentric binaries KIC 8111622, KIC 10518735, KIC 8196180 and their out-of-eclipse variability
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Light curve solutions of the eclipsing eccentric binaries KIC 8111622, KIC 10518735, KIC 8196180 and their out-of-eclipse variability

机译:Ecliping偏心二进制基金kic 8111622,kic 10518735,kic 8196180的光曲线解决方案及其外蚀变异性

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摘要

We determined the orbits and stellar parameters of three eccentric eclipsing binaries by light curve solutions of their Kepler data. KIC 8111622 and KIC 10518735 undergo total eclipses while KIC 8196180 reveals partial eclipses. The target components are G and K stars, excluding the primary of KIC 8196180 which is early F star. KIC 8196180 reveals well-visible tidally-induced feature at periastron, i.e. it is an eclipsing heartbeat star. The characteristics of the observed periastron feature (shape, width and amplitude) confirm the theoretical predictions. There are additional out-of-eclipse variations of KIC 8196180 with the orbital period which may be explained by spot activity of synchronously rotating component. Besides worse visible periastron feature KIC 811162 exhibits small-amplitude light variations whose period is around 2.3 times shorter than the orbital one. These oscillations were attributed to spot(s) on asynchronously rotating component.
机译:我们通过光曲线解决方案确定了三个偏心日落二进制文件的轨道和恒星参数。 KIC 8111622和KIC 10518735经历了总Eclipses,而KIC 8196180揭示了部分eclipses。 靶分成分是G和K星,不包括作为早期F星的KIC 8196180的主要。 KIC 8196180在Periastron中揭示了可见的神经诱导的特征,即,它是一种黯然失色的心跳明星。 观察到的PeriaStron特征(形状,宽度和幅度)的特性证实了理论预测。 具有轨道周期存在轨迹8196180的额外的异常差异,其可以通过同步旋转部件的点照射来解释。 除了较差的可见Periastron功能,KIC 811162表现出小幅度光变化,其时期比轨道上短2.3倍。 这些振荡归因于异步旋转组件的点。

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