Sometimes a neutron star results and sometimes a black hole.
有时候她也可以变为一个中子星或者黑洞。
A thimbleful of a neutron star would weigh over 100 million tons.
一颗中子星很微量的一部分，重量也会超过1亿吨。
A spinning neutron star is tied to a mysterious tail — or so it seems.
一个旋转的中子星拖出了一条神奇的尾巴，至少看起来是这样的。
One teaspoonful of material from a neutron star would weigh a billion tonnes.
一茶匙中子星上的物质重达十亿吨。
This is when the Duke team had some fun with their laser-trapped neutron star analog.
下面就是杜克大学的团队从他们的中子星激光捕捉法模拟中获得一些乐趣的时候了。
This generator drives an energetic wind of electrons and ions away from the neutron star.
这个发电机制造出强劲的能量风，把电子和离子吹离中子星。
The period of rotation of the neutron star is 0.0335028583 seconds. That's what it is today.
中子星的旋转周期,是0。0335028583秒，这是今天的数据。
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。
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。
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。
So by timing the pulses of the x-rays, you can get a handle on the Doppler shift of the neutron star.
你可以运用，中子星的,多普勒顿移，这意味着你可以得到。
Magnetars are a type of neutron star? An object so dense its protons and electrons have merged to form neutrons.
磁星是中子星的一种，它的密度非常大，其质子和电子被迫结合形成中子。
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。
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。
But they didn't have to scoop a chunk of neutron degenerate matter from the surface of a real neutron star either.
但他们也并不需要从一颗真正的中子星表面挖来一块中子星简并物质。
Magnetars are a type of neutron star which has a magnetic field a million billion times stronger than the Earth's.
磁星是一类磁场比地球磁场强千亿倍的中子星。
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。
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。
Published Wednesday in Nature, the findings make Cassiopeia's core the youngest neutron star scientists have ever encountered.
仙后座a的核心是迄今为止发现的最年轻的中子星。这一发现发表在了本周三的《自然》杂志上。
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。
So, although the researchers favor the baby black hole story over the newborn neutron star, only time and more observations will tell.
所以，虽然研究人员喜欢新生黑洞的报道甚于新生中子星，但是只有时间和更多的观察研究才能证明一切。
This neutron star was born so hot that nuclear fusion happened on its surface, producing a carbon atmosphere just 10 centimeters thick.
阿尔伯塔大学的天文学家克雷格.汉克在新闻稿中写道，“这颗中子星诞生时表面温度非常之高，以至于在它的表面也可以发生核聚变，并产生了大约10厘米厚的碳质云层。”
"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。
When constrained within the laser trap, the atoms are bunched close together, mimicking the neutron degenerate pressure of a neutron star.
当它们被激光阱束缚时，原子被捆绑并相互靠近，模拟出中子星内的中子简并压。
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 youngest known neutron star in the Milky Way, Cas a was born in a supernova explosion that astronomers may have spotted 330 years ago.
作为银河系中已知的最年轻的中子星，Cas a诞生于330年前天文学家可能观测到的一次超新星爆发中。
This would make the object in SN 1979c the youngest and brightest example of such a "pulsar wind nebula" and the youngest known neutron star.
如果是这样的话，SN 1979c中的这个天体将是迄今为止观测到的最年轻最明亮的“脉冲风星云”，是已知最年轻的中子星。
This would make the object in SN 1979c the youngest and brightest example of such a "pulsar wind nebula" and the youngest known neutron star.
如果是这样的话，SN 1979c中的这个天体将是迄今为止观测到的最年轻最明亮的“脉冲风星云”，是已知最年轻的中子星。
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