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neutron stars

网络中子星

neutron stars

网络释义

neutron stars

中子星

如果连恒星演化的最后阶段也算在内，最小的星大概是中子星 (neutron stars)，中子星是大质量恒星在临终爆炸后的一种遗物， …

例句：

One of the best possible sources for gravitational waves would be a merger between compact binary neutron stars .

观测引力波的最佳时机之一就是两颗中子星互相吞噬的过程。

A third topic is that of the high-density colour superconductive state of matter , which may be present in the core of neutron stars .

第三个议题是，在高密度色超导物质的状态，这可能是在中子星的核心存在。

He said the neutron stars can be no larger than about 20 . 5 miles (33 kilometers ) across.

他指出，这些中子星的直径不可能超过 20.5 英里（33 公里）。

To find out how strong the crusts of neutron stars really are , Horowitz and a colleague created a computer simulation of a star 's surface .

为了发现中子星的地壳到底有多么硬，Horowitz 和一位同事建立了一颗星球表面的计算机模拟程序。

Strong gravitational waves are thought to be produced by the collision of two neutron stars .

在两颗中子星星体之间的作用被认为会产生很强的重力波动。

One of the neutron stars is a pulsar; it emits radio pulses at regular intervals as it spins 45 times per second .

其中一颗为脉冲星，该脉冲星以每秒 45 周的旋频率向宇宙中发射有规律的无线电波。

Due to the existence of high viscosity in strange matter, strange stars can reach much shorter period than neutron stars.

由于奇异星有很高的粘度，它的自转周期会比中子星短得多。

People who believe in astrology or aliens may look for hidden meaning in this model of a black hole sucking neutron stars into its maw.

占星术和外星人的崇拜者可能会寻找这个黑洞吞噬中子星的模型背后的隐藏意义。

The most likely explanation for GRB050709 is that it was produced by a collision of two neutron stars, or a neutron star and a black hole .

对于 GRB050709 ，最可能的解释认为，它是两颗中子星，或者一颗中子星和一个黑洞碰撞的结果。

For M15, the HST astronomers relied on an earlier estimate of the number of neutron stars in the cluster.

对于 M15 ，哈勃空间望远镜的结论建立在早期对其中中子星数量的估计之上。

Carbon Earths might be especially prevalent in more bizarre settings , such as the environs of white dwarfs and neutron stars .

碳造地球在更异乎寻常的环境里，如中子星和白矮星周边可能会更常见。

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。

There is a positive observational and theoretical basis for believing that neutron stars and black holes follow as a result of supernovae .

中子星和黑洞则是超新星的产物，观测上和理论上的依据使我们相信这一点。

Pictured above is an artist 's illustration depicting two neutron stars spiraling in toward each other , just before they collide .

上图呈现了画家想像中两颗中子星螺旋掉向对方，在碰撞前的瞬间。

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！

Neutron stars are created when massive stars run out of fuel and collapse .

中子星是在大型恒星耗尽燃料后崩溃而产生的。

Not just any old relics, neutron stars are the leftover cores of huge stars that exploded in supernovae .

和一般残骸不同，中子星是以超新星方式爆炸的巨大星球的残余核心部分。

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。

Searching for X- ray sources in the sky becomes the most important ways to locate neutron stars and black holes among binary system .

观测星空中的 X 射线源成为寻找双星系统中的中子星或黑洞的最重要方法。

We adopt a new train of thought to constrain the equations of state of neutron stars .

我们采用一种新思路限制了中子星状态方程。

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