查询词典 pulsars

The correlation between short period and weak magnetic field of binary pulsar and millisecond pulsar implies that these pulsars are the recycled pulsars of existing binary accretion process.

双星脉冲星和毫秒脉冲星的短周期和弱磁场相关性暗示这些脉冲星是存在双星吸积过程的反加速脉冲星。

To see two pulsars orbiting each other in a binary system is extremely rare in itself.

在双星系统中看到两颗相互围绕运行的脉冲星是非常罕见的。

For example, we investigate Maxwell equation and Boltzmann equation in the above spacetime and the new properties of plasma and the theory of the radio emission of pulsars in flat spacetime.

比如，较详细地讨论了平坦空间和弯曲空间的Maxwell方程和Boltzmann方程，平坦空间中等离子体的新特性以及中子星磁层的射电辐射理论。

The purple dots represent the known pulsars, which have been detected electromagnetically.

屏保中紫色的点表示已知的通过电磁方法探测到的脉冲星。

Using three pulsars, the satellite position in the inertial frame can be resolved.

同时测量三颗脉冲星，就可以计算出卫星在惯性系下的位置。

In §3.2 we study the radio luminosity of type Ⅰ pulsars.

在§3.2我们主要计算Ⅰ型脉冲星的射电光度。

Pulsars evolving under such process are stable, and according to the magnetic field strength, this process will last as long as hundreds of years or as short as several minutes.

在这些过程中，脉冲星是稳定的，根据磁场强度的不同，这种行为会持续长则百年或者短则数分钟。

Ray emitting radio pulsars which shine on their own, there are a large number of galactic neutron stars and black holes which owe their gamma-ray light to the effect of a companion star.

与释放出v射线辐射的脉冲星自己闪烁不同，很多极大的中于星和黑洞受其伴星的影响，也释放出y射线。

Unlike gamma ray emitting radio pulsars which shine on their own, there are a large number of galactic neutron stars and black holes which owe their gamma-ray light to the effect of a companion star.

与释放出v 射线辐射的脉冲星自己闪烁不同，很多极大的中于星和黑洞受其伴星的影响，也释放出y 射线。

Only for a few pulsars one can estimate their ages with their proper motion data, it is difficult for most pulsars.

对少数几个脉冲星可以利用自行资料来估计其"动力学年龄"，而对绝大多数脉冲星则无法这样做。

In the negative and interrogative forms, of course, this is identical to the non-emphatic forms.

。但是，在否定句或疑问句里，这种带有"do"的方法表达的效果却没有什么强调的意思。

Go down on one's knees;kneel down

屈膝跪下。。。下跪祈祷