CBS HZ Her=Her X-1的光学观测
Optical Observations of the CBS HZ Her=Her X-1
摘要：
光电观测的高精度和长时间跨度使它们能够用于多因素分析和改进密近双星系统光变曲线中的一些“精细”光度效应。所得结果可以用密近双星系统光学组分到中子星吸积盘上的质量流模型来解释，它可以满意地解释气体流的不规则性、“热点”和在中子星Her X-1的吸积盘外部以单独的开普勒轨道运动的飞溅的存在。
英文摘要：
The high accuracy and long time span of photoelectric observations allow them to be used for multifactor analyses and refining some of the "fine" photometric effects in the light curves of close binary systems. The results obtained can be subsequently interpreted in terms of the model of mass flow from the optical component of the close binary systems onto the accretion disk of the neutron star, which can explain satisfactorily the irregularities of the gaseous flow, the "hot spot", and the presence of splashes moving in individual Keplerian trajectories about the outer parts of the accretion disk of the neutron star Her X-1.
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