1.【天】脉冲星
1.a type of star in space that produces a regular radio signal
1.There may be a real physical cause for dispersion of the pulsars out of the plane.
该面以外的脉冲星的弥散也许有其真正的物理原因。
2.Only a tiny fraction of pulsars is in binary systems where their masses can be determined.
而这其中只有很小一部分，因为是处在双星系统中的脉冲星，我们能够确定他们的质量。
3.To see two pulsars orbiting each other in a binary system is extremely rare in itself.
在双星系统中看到两颗相互围绕运行的脉冲星是非常罕见的。
4.The uniqueness of this class of objects and certain shared features argue in fact that all pulsars have such an origin.
这类天体的独特性质和某些共有的特点，事实上说明所有的脉冲星都有这样一种起源。
5.Searches for binary radio pulsars so far were called "acceleration searches" or "sideband searches" .
目前为止对脉冲双星的搜索都称之为”加速度搜索“或者”边频带搜索“。
6.Pulsars and Supernovae are shown on the sky because scientists believe they emit gravitational waves.
天球上标识出了脉冲星和和超新星遗迹，因为科学家们相信它们都会发射出引力波。
7.Pulsars are the dense cores left over after stars of a certain mass explode into supernovae.
脉冲星是某一恒星群发生爆炸形成超新星后所遗留下来的密核。
8.Unlike past uses of pulsars to probe gravitational waves, this technique picks up the direct effects of the waves.
这项技术不像过去是以脉冲星来探测重力波，而是筛选出重力波所带来的直接影响。
9.Pulsars can emit gravitational waves by a variety of mechanisms in the sensitive frequency range of ground-based detectors.
脉冲星能够通过多种机制发射引力波，而且正好是在地基探测器的比较灵敏的频率范围内。
10.Pulsars are widely thought to be rapidly rotating, magnetized neutron stars.
一般认为，波霎就是快速自转并且带有磁场的中子星。