论文标题
开普勒系统KIC 10661783与$δ$ scuti组成
Simultaneous binary and asteroseismic modelling of the Kepler system KIC 10661783 with the $δ$ Scuti component
论文作者
论文摘要
我们介绍了Eclipsing Binary System的分析和建模的结果，KIC 10661783。校正了针对二进制效应的开普勒光曲线的傅立叶分析，揭示了P和G模式区域的750个频率峰。振幅最高的人集中在20-30 d $^{ - 1} $的范围内。为了再现观察到的频率频谱，我们构建了占模式不稳定性的地震模型。为了在G模式制度中获取不稳定性，我们修改了Z-沉重范围附近的不透明度表数据。为了重现系统参数，我们构建了包括二进制进化的进化模型。
We present the results of analysis and modelling of the eclipsing binary system, KIC 10661783. The Fourier analysis of the Kepler light curve, corrected for the binary effects, reveals 750 frequency peaks in both p and g-mode regions. Those with the highest amplitudes concentrate in the range of 20-30 d$^{-1}$. To reproduce observed spectrum of frequencies we construct seismic models accounting for the mode instability. In order to obtain instabilities in the g-mode regime we modify the opacity tables data near the Z-bump. In order to reproduce system parameters, we construct evolutionary models including binary evolution.
