pulsars
美 [ˈpʌlsɑr] 
英 [ˈpʌlsɑː(r)]
词形变化
复数：pulsars
英汉解释
英英解释
例句
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。
A decade ago, he says, very little was known about any connections between pulsars and magnetars.
10年前，我们对脉冲星和磁星的关联知之甚少。
Some neutron stars become pulsars , stars that send off pulses of radio waves. These can also cause gravitational waves.
一些中子星变成了脉冲星，即发射电磁波的星体，它们也可能会产生引力波。
The limited sensitivity of present pulsar surveys and the greater frequency drift make the more distant pulsars difficult to observe.
目前脉冲星普查的有限探测灵敏度和大的频率漂移，使我们难以观测到更遥远的脉冲星。
In addition to extraterrestrial signals we might see signs of evaporating black holes or discover new pulsars.
除了来自外星人的信号，我们可能还会看到黑洞蒸发或者发现新的脉冲星。
Thus, a significant fraction of pulsars are being missed in the surveys.
因此，这样的调查其实错过了很大一部分的脉冲星。
This is when I concentrated on pulsars and built a large machine to do realtime processing of pulsar radio signals, right at the telescope.
这段时间我主要研究脉冲星，并建造了一台大型设备，直接在望远镜上对脉冲星射频信号进行实时处理。
Pulsars: Neutron Stars or Strange Stars?
脉冲星是中子星还是奇异星？
From this, most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss.
从这个论点来推断，大部份年轻的无线电波霎应具有介于1012~1013高斯的磁场。
The solution emerged from an entirely separate line of work, on radio pulsars .
问题的答案，得从另一条完全不相同的思路中寻找：无线电波霎。
XMM-Newton discovered X-ray emission from both pulsars in October 2006.
牛顿在2006年10月发现了来自两颗脉冲星的X射线辐射。
These are pulsars -- the dense, fast-spinning, and intensely magnetic leftovers of exploded stars.
这些脉冲星，高密度的，快速旋转的，具有强大的爆炸的恒星剩余磁力的形体。
For example, spinning neutron stars called pulsars emit clocklike streams of electromagnetic pulses.
例如，被称为脉冲星的自旋中子星发射出像钟摆一样的电磁脉冲。
speeding up in the rotational periods of binary stars and pulsars
加快了双系统星和脉冲星的旋转周期；
Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes ( Astrophysics and Space Science Proceedings )
紊乱，发电机，增长磁盘，脉冲星与等离子群过程。
Positioning for a Spacecraft using Pulsars
脉冲星在空间飞行器定位中的应用
Research Progress and developments Prospectsof millisecond pulsars timing method
毫秒脉冲星计时方法的研究进展和前景
Research on the Spacecraft Autonomous Navigation Using Pulsars
基于脉冲星的空间飞行器自主导航技术研究
Progress in the Studies of Interstellar Scintillation of Pulsars
脉冲星星际闪烁的研究进展
A Three-dimensional Outer-magnetospheric Gap Model for Crab-like Pulsars
类Crab脉冲星的三维磁层外隙模型
Research on Analysis and Processing Methods for Weak Signal and Noise of Pulsars
脉冲星极弱信号和噪声分析与处理方法的研究
