RESULTS OF 40-YEAR STUDIES OF THE X-RAY BINARY CYG X-1=V1357 CYG

被引：0

作者：

Karitskaya, E. A. ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Astron, Pyatnitskaya Str 48, Moscow 119017, Russia

来源：

BALTIC ASTRONOMY | 2016年 / 25卷 / 01期

关键词：

stars:; atmospheres; abundances; accretion disks; individual; (V1357; Cyg); X-rays: binaries; ELECTRON-SCATTERING ATMOSPHERES; TIDALLY DISTORTED STARS; X-1; V1357; CYG; PROJECTIONS ASTROTOMOGRAPHY; INTRINSIC RADIATION; INTERSTELLAR MATTER; STATE TRANSITIONS; MAGNETIC-FIELD; BLACK-HOLE; POLARIZATION;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper reviews the results of our 40-year studies of Cyg X-1 using various methods and observational data: mainly optical photometric, spectroscopic, and polarimetric ones, with X-ray data also considered. We show that, while performing model calculations approximating observational data, it is vital to take into account a diversity of factors, for example, the accretion structure variations that influence the shape of the orbital light curve. We emphasize the necessity of comprehensive studies, development and usage of all possible methods.

引用

页码：89 / 106

页数：18

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