论文标题
接触二进制系统NSVS 2983201的研究
A study of a contact binary system NSVS 2983201
论文作者
论文摘要
在这里，我们介绍了短期可变星NSVS 2983201的观察结果和第一光曲线分析。使用光曲线数值建模，我们发现最佳拟合模型是浅的（FF = 10％）接触质量比质量比Q = 0.36。系统的光曲线具有O'Connell效应，从而识别出较大的圆形星点。通过仔细的多箱分析，我们搜索系统的物理参数。我们发现使用不同方法获得的结果要接近，但不重叠。该系统将安排进一步监视。
Here we present the observations and the first light curve analysis of the short-period variable star NSVS 2983201. Using the light curve numerical modeling we find the best fitting model to be of shallow (ff=10%) contact binary configuration of mass ratio q=0.36. The light curve of the system experiences the O'Connell effect, which led to identifying a large circumpolar starspot. With a careful multi-cases analysis we search for the physical parameters of the system. We find the results obtained with the different methods to be close, but not overlapping. This system will be scheduled for the further monitoring.
