Photometric solution of the eclipsing binary system EF Boötis
Photometric solution of the eclipsing binary system EF Boötis
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DOI：
10.1002/asna.200310174
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发表时间：
2004-05
影响因子：
0.9
通讯作者：
S. Ozdemir;O. Demircan;C. Çiçek;A. Erdem
中科院分区：
文献类型：
--
作者：
S. Ozdemir;O. Demircan;C. Çiçek;A. Erdem
在文献发表的光学光曲线和径向速度曲线的背景下，研究了EF BOO食双星系统。最佳解决方案导致WUMA系统的W子类过接触配置，填充系数为28%。给出了基于光速曲线和径向速度曲线同时求解的绝对参数。(2014Wiley-VCH Verlag GmbH&Co.KGaA，Weinheim)
The EF Boo eclipsing binary system is studied in the context of optical light curves and radial velocity curves published in the literature. The best-solution leads to an over-contact configuration of W–subclass of WUMa systems with a fill-out factor of 28%. Absolute parameters based on simultaneous solution of light and radial velocity curves are presented. (© 2004 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)