脉冲星的例句大全

The present and potential situation of the pulsar observation research in China is analysed.

分析了我国脉冲星观测研究的现状和潜力、存在的问题和美好的前景.

They discovered a new pulsar wake.

他们发现了一个新的脉冲星尾迹.

A nuclear waste dump at the South Pole might actually be a little more pleasant.

南极的核垃圾站可能都比脉冲星好些。

A three-dimensional model of the pulsar magnetosphere by Prof K . S . Cheng of HKU.

脉冲星磁层的三维模型﹝照片提供:香港大学郑广生教授﹞.

We use a three dimensional pulsar magnetosphere model to study the geometry of outer magnetospheric gaps.

利用三维脉冲星磁层模型研究了磁层外隙的几何结构.

Its properties implied from pulsars, X-ray binaries and gamma-ray bursts are discussed.

脉冲星、X射线双星以及γ射线爆源，都可能存在着这种第二类磁场。

For example a pulsar is a rapidly spinning neutron star with a strong magnetic field.

例如,脉冲星是具有强大磁场和高速旋转的中子星.

One possibility is pulsars – rotating neutron stars that emIt'strong radio transmissions.

一种可能就是脉冲星——不停发出强大电磁波的旋转中子星.

Rotating Rigid Bodies-Moment of Inertia-Parallel Axis and Perpendicular Axis Theorem-Rotational Kinetic Energy-Fly Wheels-Neutron Stars-Pulsars.

刚体的转动-转动惯量 - 平行转轴定理和垂直转轴定理 - 转动动能 - 飞轮 - 中子星-脉冲星.

Last year, astronomers at the National Radio Astronomy Observatory in Charlottesville, Virginia, discovered the first pulsar orbited by two other shrunken stars, called white dwarfs.

去年在弗吉尼亚州夏洛茨维尔，国家射电天文台（National Radio Astronomy Observatory）的天文学家发现了一颗脉冲星，绕着它运动的另外两颗缩小的恒星被称为白矮星，而这一现象是前所未见的。

Pulsars, neutron stars and quark stars are then created based on their mass.

因质量的大小而形成脉冲星 、 中子星、夸克星,质量大到一定值的生成黑洞.

Supernovae remnants can leave behind pulsars or spinning neutron stars that may produce gravitational waves.

超新星遗迹中可能还存留有脉冲星或自旋中子星,而这些都会产生引力波.

The cooperation program between China, Australia and Great Britain, Pulsar timing observation at 18 cm using 25 m radio telescopy of Urumqi, is introduced for its significance, reconstruction of the receiver and its sensitivity.

对正在执行的由中、澳、英合作的利用乌鲁木齐25m射电望远镜在18cm波段上进行脉冲星脉冲到达时间的观测研究项目，就其课题意义、接收系统的技术改造和观测灵敏度等进行了介绍。

This paper touches the progress in VLBI astrophysics concerning some high lights of extragalactic continuum astronomy, interstellar masers and pulsars and stars from VLBI observations.

本文评述VLBI天体物理学的进展，特别是在河外连续谱天文学、星际脉泽、脉冲星和恒星等方面VLBI观测的主要结果。

The comparisons between the frequency stabilities for atomic time and pulsar time are presented.

给出了毫秒脉冲星长期计时观测最新结果和脉冲星时与原子时频率稳定度的比较.