论文标题
在黯淡的二进制文件中具有椭圆轨道的第三个组件：BD和SV CAM，V0836 CYG和XZ CMI
Third components with elliptical orbits in the eclipsing binaries: BD and, SV Cam, V0836 Cyg & XZ CMi
论文作者
论文摘要
这是我们在循环O-C变化和第三个组件领域的定期研究。在本文中，描述了四个新恒星调查的结果。这些恒星是：BD和SV CAM，V0836 CYG和XZ CMI。它们都具有线性（BD和SV CAM和XZ CMI）或抛物线趋势（V0836 CYG）的环状O-C曲线。我们计算了每个研究恒星的传质率，最小值质量及其误差。
This is our regular research in the field of cyclic O-C changes and third components. In this article the results of four new stars investigation is described. These stars are: BD And, SV Cam, V0836 Cyg and XZ CMi. All of them have cyclic O-C curve with linear (BD And, SV Cam and XZ CMi) or parabolic trend (V0836 Cyg). We computed the mass transfer rate, minima possible mass of the third component and their errors for each of the researched stars.
