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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:遮蔽偏心双星KIC 8111622的光线曲线解决方案,   KIC 10518735,KIC 8196180及其日食变异性

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摘要

We determined the orbits and stellar parameters of three eccentric eclipsingbinaries by light curve solutions of their Kepler data. KIC 8111622 and KIC10518735 undergo total eclipses while KIC 8196180 reveals partial eclipses. Thetarget components are G and K stars, excluding the primary of KIC 8196180 whichis early F star. KIC 8196180 reveals well-visible tidally-induced feature atperiastron, i.e. it is an eclipsing heartbeat star. The characteristics of theobserved periastron feature (shape, width and amplitude) confirm thetheoretical predictions. There are additional out-of-eclipse variations of KIC8196180 with the orbital period which may be explained by spot activity ofsynchronously rotating component. Besides worse visible periastron feature KIC811162 exhibits small amplitude light variations whose period is around 2.3times shorter than the orbital one. These oscillations were attributed tospot(s) on asynchronously rotating component.
机译:我们通过开普勒数据的光曲线解确定了三个偏心日食双星的轨道和恒星参数。 KIC 8111622和KIC10518735经历了全月食,而KIC 8196180则出现了部分日食。目标成分是G和K星,不包括早期F星KIC 8196180的主要星。 KIC 8196180揭示了潮汐加速器中可见的潮汐诱发特征,即它是一颗黯淡的心跳星。观测到的围星体特征(形状,宽度和幅度)的特征证实了理论预测。 KIC8196180随轨道周期还有其他的蚀外变化,这可以通过同步旋转分量的点活动来解释。除了较差的可见周星光特征,KIC811162还显示出幅度较小的光变化,其周期比轨道周期短约2.3倍。这些振荡归因于异步旋转组件上的一个或多个点。

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