分散在超大质量黑洞周围的中子星。
这也是实验得以类比中子星物质的地方。
This is where the experiment becomes analogous to the material of a neutron star.
现在我只讲，这个中子星。
For now, I just want to concentrate on this neutron star alone.
科学家发现的其他中子星均要比这颗更老。
Every other neutron star identified by scientists has been much older.
中子星旋转的计时，如果中子星。
这个中子星，由于它不是很好理解，正向我们闪耀。
This neutron star for reasons that is not well understood is blinking at us.
最后，我们研究了中子星的质量和半径。
中子星继续缩小，直到它变成一个黑洞。
The neutron star continues to shrink until it finally becomes a black hole.
对着中子星久了，也就研究出一些心得。
Toward neutron star Be getting longer, also study a some insights.
这就是中子星。
新发现的这颗中子星只有单一的碳大气层，厚十余厘米。
The newly identified neutron star has a unique atmosphere of carbon just centimetres thick.
然而，太阳与中子星一起就会有些不同寻常。
其次，我们研究了零温时中子星物质的物态方程。
Secondly, the equation of state of neutron matter at zero temperature is studied.
然而，至于它到底属于哪一类中子星，仍然是个谜。
Exactly which type of neutron star it is, however, remains a mystery.
对于大多数这样的星球来说，星球核心最终会变成一颗中子星。
For most such stars, the core is left behind as a neutron star.
我们知道，这些物体是存在的，因为使用射电望远镜已经观察到了几个中子星。
We know that these objects exist because several have been found using radio telescopes.
我们知道，这些物体是存在的，因为使用射电望远镜已经观察到了几个中子星。
We know that these objects exist because several have been found using radio telescopes.
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