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pulsars

美 [ˈpʌlsɑr]英 [ˈpʌlsɑː(r)]

n.【天】脉冲星
网络波霎；研究脉冲星；脉冲中子星

复数：pulsars

pulsars

pulsars

英-汉英-英网络释义

pulsars

n.

1.【天】脉冲星

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。

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。

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。

11

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？

13

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。

14

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。

16

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！

17

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。

18

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。

19

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。

20

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。

21

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。

25

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。

27

Pulsars: Neutron Stars or Strange Stars ?

脉冲星是中子星还是奇异星？

28

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。

30

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。

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