X-ray binary

The Study of Be / X-ray Binary Envelope

Be/X射线双星包层性质的研究

Spectral study of be / x-ray binary lsi + 61 ° 303

Be/X射线双星LSI+61°303的光谱研究

Perhaps the first object to be generally recognized as a black hole is the X-ray binary star Cygnus X - 1 .

也许最早被普遍认为是黑洞的物体，是发射X射线的双星天鹅座X－l。

An X-ray binary system has been formed , and the neutron star has made the crucial second step toward becoming a millisecond pulsar .

射线双星就这样形成了，于是这颗中子星就向成为毫秒脉冲星迈出了关键的第二步。

Cygnus X-1 is an x-ray binary which has an orbital period of5.6 days .

双星，轨道周期是，5。6天，进行对供体星的。

What we studied includes the envelopes of Be stars , the nature of the stellar wind , formation mechanism and Be / X-ray binary material interaction etc.

研究内容包括Be星包层和星风的性质，以及包层形成机制，Be/X射线双星物质相互作用等。

Recent years , the careful and systematical analyses of the observational data about pulsars and the evidences provided from the observations of millisecond pulsars , radio and X-ray binary pulsars have posed more and more problems on the formation , evolution and radiation mechanisms of pulsars .

近年来，对日益增加的脉冲星观测资料的分析和对毫秒脉冲星、射电和X射线脉冲双星的观测，对脉冲星的形成、演化和辐射机制等提出了越来越多的新问题。

This paper is contributed to the study of the light curve and periodicity of the black hole X-ray binary Cyg X-1.Black hole is the high-mass compact object , which is result of the gravity collapse of the star and most of the black hole system is X-ray nova .

本文主要致力于黑X射线双星光变曲线以及周期性特征的研究。黑洞是经过恒星引力塌缩而形成的一种质量较大的致密天体，几乎所有的黑洞系统是X射线新星。

The X-ray source in binary stars and the spin down of neutron stars

双星X射线源与中子星的自转减速

This highlights the critical importance of high-resolution observations at high X-ray energies in locating binary AGN .

这显示在二进制活动星系核的定位在高X射线能量高清晰度观测至关重要。

Both theoretical and experimental results showed that linear calibration curve could be obtained if the curve is plotted by Re % vs. ReL α x-ray intensity instead of binary ratio technique .

理论和实验结果均表明：直接用ReLα分析线强度绘制的校正曲线比二元比例法可以获得更好的线性。