neutron star
美 
英
- na.【天】中子星
- 网络成中子星；脉冲星中子星；中子星座
英汉解释
英英解释
例句
In the nebula's very center lies a pulsar: a neutron star as massive as the Sun but with only the size of a small town.
在星云的正中心有一个脉冲星：一个中心星，它拥有和太阳类似的质量而只有一个小村庄那么大。
(Kusenko likens it to "a bullet passing through a cloud of vapor. " ) And if it runs into a neutron star?
（Kusenko把这比作“一颗子弹穿过一层蒸汽”）那么它跑进中子星会发生什么呢？
Badenes's team examined archival observations and found a white dwarf and neutron star orbiting one another extremely closely.
Badenes的团队试验档案观测并发现白色小的中子星体非常近的围绕另一个运转。
And this really changed our whole concept of astronomy, the existence of these neutron star binaries.
对于天文学的概念，这些中子双星的，存在，现在一部分是。
And I take a little bit of matter m, and I drop it from a large distance onto the neutron star.
从很远的距离扔到，中子星上，那个小物体。
Astarquake is thought to be the tearing apart of the surface of a neutron star, much like an earthquake here on Earth.
恒星地震拒信可以撕裂中子星表面，其所能产生的破坏力很像地球上的地震。
It was the first time that astronomers have measured the rate of cooling of a young neutron star.
这是天文学家第一次测量到了年轻中子星的冷却速率。
However, you will never see pulsations, because a black hole has no surface, like a neutron star.
你将不会看到脉动，因为黑洞没有表面，它不像中子星，不存在两个热点可以。
Now, two teams of physicists say they have more direct evidence for superfluidity in the heart of a neutron star.
现在，两个小组的物理学家宣称他们掌握了中子星核心中超流的更直接的证据。
A ten-gram object thrown onto a neutron star-- the reason being that this velocity becomes enormously high.
原因就在于-，速度，变得无穷大，若扔到中子星的物体。
and ensuing explosion would blow off the outer envelope of the star and leave behind the core as a neutron star.
按此模型，引起的突然压缩和随后的爆发会把恒量的外部包层吹跑，留下的核成为一颗中子星。
Smolin's predictions, including ideas about cosmological inflation and the mass of the heaviest stable neutron star, have held up so far.
Smolin的预测，包括宇宙暴胀学说和最重稳定中子星的质量都有待验证。
After the supernova, the leftover matter could either have collapsed into a black hole or an extremely dense neutron star.
超新星爆发以后，剩余的物质可能塌缩为一个黑洞，也可能形成一颗密度极大的中子星。
In theory, the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova.
理论上，形成一颗毫秒脉冲星的第一步，是一个大质量恒星在成为超新星而爆发后留下的中子星。
It might therefore seem like an easy task to create a 'neutron star' at home.
因而看来在家里制造一个“中子星”也似乎是一个简单的活。
If the neutron star is too large, the gravitational forces overwhelm the pressure gradients and collapse cannot be halted.
如果中子星太大，吸引力胜过气压梯度，塌陷便不能被阻止。
At this point, a neutron star pair, or even a neutron star-black hole pair, is formed.
此刻，一个双中子星、甚至中子星-黑洞对将形成。
This seemingly gentle structure also harbors a very powerful spinning neutron star that may be the central remnant from the initial blast.
这些外表柔和的结构也蕴藏着一个很强大的旋转的中子星，那可能是来自最初爆炸的灰烬的中心。
Three years later, Salla's nav computer malfunctioned and deposited her vessel on a collision course with a neutron star.
三年后，萨拉的飞船因导航电脑故障，锁定航线向一颗中子星撞去。
And you don't really ; have to be infinitely far away; you just have to be much further away than the radius of the neutron star.
从无穷远处来，你只要在远大于；，中子星半径的地方，当物体撞到。
The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.
在中子星或黑洞伴星上发生吸积的模型，仍应看成是一个有价值的假说。
The only things more dense are black holes, as a teaspoonful of neutron star matter would weigh about 100 million tons.
比它密度再大的就只有黑洞了，只需要一勺匙中子星的质量就可以达到100万吨。
Basically, a black hole is formed when a very, very large star has a supernova event which can result in a neutron star or a black hole.
基本上，黑洞都脱胎于恒星，如果这颗恒星爆发成一颗非常，非常硕大的超新星，那么就可能会产生中子星或黑洞。
Since a 7-solar-mass is too large to be a white dwarf or neutron star, it must be a black hole.
因为有着7个太阳质量的星体不可能是白矮星或中于星，所以它一定是黑洞。
Such "pulsar glitches" likely result from brief interactions between the neutron star's solid crust and superfluid interior.
这种“脉冲星故障”很可能源于中子星坚硬的地壳与超流内部的短暂作用。
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。
The other neutron star does not beam radio pulses toward Earth, so it remains unseen except for its gravitational influence.
另外一颗中子星没有发出朝向地球的脉冲信号，所以除了重力影响，它不能被观测到。
Properties of nuclear matter and neutron star are described in relativistic mean field theory with density-dependent effective interactions.
基于密度相关有效相互作用的相对论平均场理论，研究了核物质和中子星的性质。
In this case, you have to open and close it with exactly the same frequency as the rotation of the neutron star.
在这个例子里，你必须以和中子星，旋转相同的频率，对其进行开关。
The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.
在中子星或黑洞伴星上发生吸积的模型，仍应看成是一个有价值的假说。
The explosion could also cause a neutron star or result in the formation of a black hole 1300 light years from Earth, reports news. com. au.
au的报道称，爆炸还会形成一个中子星（neutronstar），或者是一个距地球1300光年的黑洞。
These binary systems consist of a neutron star orbiting around a supergiant star.
这些双星系统由一个巨星和围绕其的中子星组成。
Each star of the closely-packed system is a dense neutron star, spinning extremely fast, radiating X-rays in pulses .
这个紧密系统的每一颗星都是致密的中子星，自旋非常快，辐射着X射线脉冲。
Frequent Space Museum visitors should know that neutron star is one of the possible final products of stellar evolution.
经常参观太空馆的人该知道，中子星是恒星演化至末期的结果之一。
Now, two teams say they have direct evidence of such bizarre "superfluidity" in a neutron star, and other researchers seem convinced.
现在，两个小组宣称他们掌握了这种中子星内奇异超流体的直接证据，并且其他研究者似乎相信这一发现。
A millisecond pulsar is a super compact neutron star, whose spin is highly accelerated by mass transferred from a companion star.
毫秒脉冲星是密度极大的中子星，其旋转被从伴星转移来的的物质大大地加快了。
When the neutron star moves behind the donor star, all the x-rays are absorbed by the donor star and you get x-ray eclipses.
后面移动，所有的x射线都会被，供体星吸收，得到x射线食，换句话说。
''This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimetres thick. ''
“这颗中子星产生时温度如此之高，其表面还在进行核子融合，从而产生了只有10厘米厚的碳大气层。”
As a black hole or neutron star destroys a star, tremendous amounts of radiation are released.
当黑洞或中子星将一颗恒星毁灭时将会产生巨大的辐射。
At what distance from the neutron star's surface is the radiation created that the radio observatories detect?
我们观测到的射电信号是在离中子星表面多远的距离上生成的？
A supernova can leave behind a dense, rapidly spinning core made almost completely of neutrons , called a neutron star.
超新星爆发后可能会留下一个极高密度、快速旋转的、几乎完全由中子构成的核心，即中子星。
