binary star

Binary star ( two stars that revolve around a common centre )

双星（环绕一共同中心旋转的两颗星）。

The orbit determination of visual binary star with mean anomaly

从平近点角决定目视双星轨道要素T和P的一种方法

Researchers realized that they were actually seeing a binary star system .

研究人员们意识到他们实际上是在观察一颗双子星系统。

Some Problems About the Aberration and " Binary Star Paradox "

有关光行差与双星矛盾的几个问题

Stars turning round each other form a binary star

由彼此环绕的两个星组成双星

The most convincing evidence of black holes comes from research into binary star systems .

黑洞最有说服力的证据来自对双星系的研究。

Establishment and improvement of the initial orbit of the visual binary star ads 8630

目视双星ADS8630的初轨决定和轨道改进的一种结果

On the binary star system of geostationary satellites

关于地球同步卫星的双星系统

A binary star is a double star , consisting of two stars turning round each other .

双星是两颗星，是由相互围绕旋转的两颗星组成。

For example , some accretion disks in binary star systems occasionally undergo large , temporary increases in luminosity .

例如，有些双星系统里的吸积盘，偶尔会短暂地大幅增加亮度。

The hyperbolic orbit of and its mass the visual binary star ADS9446 is determined as an example .

作为例子，我们计算了目视双星ADS9446的双曲线轨道。

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。

Configuration of the Polytropic Model of Binary Star and Its Perturbation Influence on the Orbital Elements of the Synchronous Components in Close Binary System

双星多方模型的形状及其对同步子星轨道要素的摄动影响

In some binary star systems , gas escapes from one star and is captured by the gravity of the other to form a disk .

某些双星系统中，当从一个恒星逃出的气体被另一个星体的重力捕获时，也会形成盘状结构。

A binary star is a system in which two stars revolve around each other ; a binary compound ; the binary number system has two as its base .

双星是一个由彼此环绕的两个星组成的系统；二元混合物；二进制的二进制的或与之有关的。

It 's name is Eta Carinae . It 's a star or to be absolutely accurate a binary star .

它的名字是船底座伊塔星，它是一颗恒星-或绝对准确地-双星。

It is shown that long-time implication of the " binary star paradox " in the question of aberration is a conceptive confusion .

本文指出，在光行差问题上长期纠缠住双星矛盾是概念上的混淆。

Mark ⅲ stellar interferometer and Infrared Spacial Interferometer ( ISI ) have brought a few encouraging results for binary star measurements and circumstellar shell observations .

美国MarkⅢ恒星干涉仪和红外干涉仪ISI已经在双星和拱星壳的观测方面取得了令人鼓舞的观测成果。

A spectroscopic binary star , 245 light-years from Earth , one of the brightest stars in the sky and the brightest star in the constellation Virgo .

一种用分光镜观察的距地球245光年双星，是天空中最亮的恒星之一，也是处女座中最亮的星星。

This may be a precursor of what astronomers refer to as the common envelope phase , a short-lived period of a binary star 's existence that is thought to last for just a few thousand years .

这可能是天文学家们提到的共包层阶段的前身，这是双星生命中的短期阶段被认为仅持续几千年。

This observation is the first to definitively identify binary neutron star collisions as a source of short gamma-ray bursts .

这次观测首次为中子星合并可产生伽马射线短暴给予了确凿证据。

This discovery is the first verification of a " kilonova " explosion , confirming binary neutron star collisions as one source for the universe 's heaviest elements , such as gold and uranium .

这次发现首次证实了“千新星”爆炸，确认了双中子星合并是宇宙中最重的元素的来源之一，比如金和铀。