pulsars

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。

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。

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。

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。

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“。

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。

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。

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。

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。

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。

Will it detect new pulsars, black holes, or perhaps some novel natural phenomenon of which we have no inkling?

还是新的脉冲星、黑洞或者甚至是我们一点概念也没有的新奇自然现象呢？

Pulsars and supernovas seem to take over at about 9: 00 and are truly spectacular.

脉冲星和超新星似乎在大约900的位置上，而且确实相当壮观。

Astronomers keep discovering new noisemakers in space: colliding black holes, glitching pulsars, gamma ray bursts.

天文学家仍然致力于寻找太空中新的声源：黑洞碰撞，脉冲星干扰，伽马射线爆破。

When pulsars, as they became named, were discovered in the 1960s, they were nicknamed LGM for "little green men. "

脉冲星发现并命名于20世纪60年代，当时获得了LGM（小绿人）的绰号。

Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation.

脉冲星是旋转磁中子星，发出肉眼可见的电磁辐射。

However, we should be aware that pulsars may not be neutron stars at all, they may be Strange Stars!

然而，脉冲星有可能根本就不是中子星，而是由奇异物质构成的、具有很高奇异数的奇异星！

Radio pulsars are neutron stars with an immensely strong magnetic field.

射电脉冲星是带有强磁场的中子星。

The purple dots represent the known pulsars , which have been detected electromagnetically.

屏保中紫色的点表示已知的通过电磁方法探测到的脉冲星。

This procedure doesn't work as well for pulsars in most short-period binary systems.

这个过程对大部分短周期的双星系统来说效果并不好。

Interest was renewed in the astronomical community with the discovery of pulsars .

天文学团体随着脉冲星的发现重新激发了兴趣。