毫无疑问，在这个，旋转中子星的例子里，所有辐射的能量，都是以旋转动能，为代价。
So there's no question that in the case of this rotating neutron star, all the energy that it radiates is at the expense of rotational kinetic energy.
图片靠近中心部分的白色光源为一种密度大，急速旋转的中子星，或是脉冲星--都是核心坍缩的超新星爆炸的残留物。
The white source near the center of the image is a dense, rapidly rotating neutron star, or pulsar, all that remains of a core-collapse supernova explosion.
脉冲星是快速旋转的中子星，它向周围的太空抛射出能量，制造出复杂和有趣的结构，这个类似于太空巨手的结构便是其中之一。
The pulsar is a rapidly spinning neutron star which is spewing energy out into the space around it to create complex and intriguing structures, including one that resembles a large cosmic hand.
然而，如果考虑旋转动能，情况就不同了，因为这个中子星，旋转一周是33毫秒。
However, if you look at rotational kinetic energy, the situation is very different, because this neutron star rotates in 33 milliseconds about its axis.
这幅图像中还包含了几个神秘的X-射线片断，它们中的一些可能是因为巨大的磁场结构和强电子流相互作用而产生了快速旋转的中子星。
The image also contains several mysteriousX-ray filaments, some of which may be huge magnetic structuresinteracting with streams of energetic electrons produced by rapidlyspinning neutron stars.
我昨天打电话问我，射电天文学的朋友，中子星在蟹状星云的，旋转周期是多少。
I called my radio astronomy friends yesterday and I asked them, "What is the rotation period of the neutron star in the Crab Nebula?"
中子星的旋转周期,是0。0335028583秒，这是今天的数据。
The period of rotation of the neutron star is 0.0335028583 seconds. That's what it is today.
脉冲星是已经死亡的小型中子星，直径只有20公里(12.4英里)左右，每秒旋转数百次，同时还会向外发出无线电光束。
Pulsars are tiny, dead neutron stars that are only around 20 kilometers (12.4 miles) in diameter and spin hundreds of times a second, emitting beam of radiation.
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。
A spinning neutron star is tied to a mysterious tail — or so it seems.
中子星旋转的计时，如果中子星。
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。
In this case, you have to open and close it with exactly the same frequency as the rotation of the neutron star.
给你供体星的概念，然后是物体的旋转，它旋转，终止于中子星上，这里你看到的是。
And this is another view that gives you an idea of the donor and then the swirl of matter, and then it swirls in and ends up here on the neutron star.
脉冲星的结构。一颗旋转磁中子星。
脉冲星是快速旋转的中子星是进入太空的能量喷涌围绕它来创建复杂而有趣的结构，包括一个类似于一个大宇宙的手。
The pulsar is a rapidly spinning neutron star which is spewing energy out into the space around it to create complex and intriguing structures, including one that resembles a large cosmic hand.
是强有力的x射线源，中子星绕中心旋转。
不合这两点之间的线，相一致，如果中子星旋转，你会看到x射线脉动，当热点在这里。
And if the axis of rotation doesn't coincide with the line through the two hot spots, if the neutron star rotates, you're going to see X-ray pulsations.
脉冲星是旋转磁中子星，发出肉眼可见的电磁辐射。
Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation.
结果发现，质量、红移及旋转频率对相应状态方程质量-半径关系的简单限制很难区分不同的中子星模型。
We discover that it is hard for us to distinguish different neutron star models by the simple constraints of masses, redshifts and rotations on mass-radius relations.
PSRJ0737-3039包含一颗旋转稍慢“懒惰”的中子星（脉冲星B）围绕着一颗旋转较快也更活跃的同伴（脉冲星A）。
PSR J0737-3039 contains a slowly-rotating 'lazy' neutron star (pulsar B) orbiting a faster and more energetic companion (pulsar A).
这些外表柔和的结构也蕴藏着一个很强大的旋转的中子星，那可能是来自最初爆炸的灰烬的中心。
This seemingly gentle structure also harbors a very powerful spinning neutron star that may be the central remnant from the initial blast.
被认为是它的点源模型有：太阳、超新星爆发、白矮星和脉冲星（告诉旋转的中子星）等。
Up to now, there are not definite source models of cosmic rays though they come from the Sun, supernovas' explosion, the white dwarfs and pulsars, et al.
在这些程序的帮助下，我们能够确定旋转如何改变了中子星的性质，及其形状，还有对旋转的限制。
With helps of the codes we can therefore determine how rotation changes the properties of the star, the shapes of the star, also the limitation of rotation.
如果这样，这两颗高速旋转的中子星或脉冲星将会是天空中最明亮的物体。
If you could, these two spinning neutron stars or pulsars would be among the brightest objects in the sky.
如果这样，这两颗高速旋转的中子星或脉冲星将会是天空中最明亮的物体。
If you could, these two spinning neutron stars or pulsars would be among the brightest objects in the sky.
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