accretion by neutron star.
中子星吸积
Accretion of a Neutron Star Moving at a High Kick Velocity in Supernova
宝马高速腾越超新星中高速中子星的吸积
The Spontaneous Broken Symmetry and Acoustic Speed in The Neutron Stars
中子星中的对称性自发破缺与声速
The most plausible hypothesis is that the shortduration 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。
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。
But why would a neutron star behave like this
可是为什麽中子星会有这种行为呢？
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。
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。
Influence of chiral symmetry spontaneous breaking on neutron star
手征对称性自发破缺对中子星的影响
Study of Bulk Viscosity of Neutron Stars.
中子星整体粘滞性的研究
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。
Then the white dwarf will collapse and becomes a neutron star.
变成个中子星，当我们测量中子星的。
If a core continues collapsing beyond the neutron star stage, it may become a black hole.
如果中子星再进一步蹋缩, 它将可能成为一个黑洞。
Before the two neutron stars collide, they would orbit each other as a binary system.
两颗中子星相撞前, 它们必然是一对互相绕转的双星系统。
Does a neutron star represent the ultimate in compression ?
中子星是压缩的最终产物吗？?
Conversion of neutron stars to strange stars.
从中子星到奇异星的转变
Response of the Neutron Star Properties to the Equation of State at Low Density
低密度物态方程对中子星性质的影响
Describing Neutron Stars with the Relativistic Mean Field Theory
中子星的相对论平均场描述
Determining the Mass of a Neutron Star
决定中子星质量
Gas from the dwarf flows into a hot spiraling disk around the neutron star.
气体从矮星流入一个绕中子星旋转的炽热的吸积盘中。
Effect of Temperature on Hyperon Neutron Star
超子中子星性质的温度效应
Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation.
脉冲星是旋转磁中子星，发出肉眼可见的电磁辐射。
Study of the Gravitational Energy in Neutron Stars
中子星内引力能的研究
A tengram 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。
Equation of State and Proton Ratio on the Inner Shell Layer of Neutron Stars
中子星内壳层的物态方程和质子丰度
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