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Pulsars: Neutron Stars or Strange Stars? 脉冲星是中子星还是奇异星?
Hubble sees a neutron star all alone in space. 由哈勃望远镜在太空中观测到的一颗孤单的中子星。
But why would a neutron star behave like this? 可是为什麽中子星会有这种行为呢？
Are some known neutron stars actually strange stars? 一些已知的中子星会否就是奇异星?
Does a neutron star represent the ultimate in compression? 中子星是压缩的最终产物吗?
A sudden change in the period of rotation of a neutron star. 中子星旋转周期的突然变化
There also have gamma-rays emitting from black holes and neutron stars. 同样，黑洞和中于星也能够释放出v射线。
Neutron superfluid vertex in neutron stars is discussed in this paper. 摘要讨论了中子星内中子超流涡旋。
Neutron stars are the second exhibit in the gallery of stellar corpses. 中子星是死之恒星陈列馆内第二类样品。
The properties of neutron stars are investigated in the frame work of RMF. 利用我们改进的相对论平均场理论对中子星的性质进行了深入研究。
The strong gravitational field of a neutron star provides the answer. 中子星的超强引力提供了最佳的解答。
Supernovae remnants can leave behind pulsars or spinning neutron stars that may produce gravitational waves. 超新星遗迹中可能还存留有脉冲星或自旋中子星，而这些都会产生引力波。
The most plausible hypothesis is that the short-duration bursts arise from a merger of two neutron stars. 最可能的假说认为，短爆是由两个中子星合并而引起的。
X-ray flashes had previously been detected from some neutron stars, but they never exceeded the Eddington limit by very much. 以往天文学家就曾观测到过从中子星发出来的X射线闪光，但其亮度从来不会超过艾丁顿上限太多。
The former happen when an old neutron star spirals to its death in a preexisting black hole. 在一颗老迈的中子星渐渐死亡，落入一个业已存在的黑洞中时，前一种情况也就发生了。
One ramification of our calculations is that radio pulsars are neutron stars in which the large-scale dynamo has failed to operate. 从我们的计算中，还可以附带得到一点：无线电波霎正是无法形成大尺度发电机的中子星。
The bright source at the center of the image is presumed to be a neutron star created during the supernova. 图片中心的明亮辐射源据信是超新星爆发过程中产生的中子星。
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。
Astronomers knew several examples of neutron stars that lie within supernova remnants. 天文学家早就知道好些个位在不同超新星残骸里的中子星。
Once the mass is found, it can be determined if the candidate is a neutron star or a black hole. 一旦获得了质量，就可以判断这个候选体是中子星还是黑洞。