When the beams sweep across the Earth, they can be heard as regular pulses, so we call them pulsars.

当它们扫过地球时，我们会接收到有规律的脉冲，因此它们被称作脉冲星。

Each golden record displays the location of our solar system with respect to fourteen pulsars.

每个金唱片都显示着我们太阳系相对于14个脉冲星的位置。

And the second big thing is pulsars and things going bang in the sky.

第二件大事是脉冲星和空中爆炸的物体。

The other end of our detector is these pulsars that are about 3000 light years away from us

探测器的另一端是距离我们大约 3000 光年的脉冲星。

But Ig and Rev were big helps in finding previously unknown pulsars in our own Milky Way galaxy—24 of them.

但是这些网友在找到银河中之前未知的24颗脉冲星发挥了很大作用。

They also used it to find an unusual kind of star system, a binary pulsar, in 1967.

1967年，科学家还用该望远镜找到了一个罕见的恒星系统，即脉冲双星。

She had discovered the first known pulsar.

她发现了第一颗脉冲星。

Pulsars have such extreme gravity because they're made of incredibly dense matter.

脉冲星之所以有如此强劲的引力，是因为构成它的物质非常致密。

Telltale tweaks to the spins of dead stars called pulsars scattered throughout the Milky Way.

散布在银河系中的、被称为“脉冲星”的死亡恒星，其自转发生了微妙的变化。

Some of them we see as pulsars, flashing in brightness as they spin.

其中一些在我们看来是脉冲星，在旋转时闪烁着明亮的光芒。

Discovered in 1967, pulsars spin very rapidly, often hundreds of times per second.

脉冲星于1967年被发现，它们的转速极快，往往每秒钟能旋转数百周。

And we time an array of pulsars will look for gravitational wave signals.

我们计算脉冲星阵列寻找引力波信号所用的时间。

Yeah. So the term pulsar timing array implies we're timing these pulsars.

好的。“脉冲星计时阵列”这个词意味着我们在为这些脉冲星计时。

" We think this new signal could be a magnetar or pulsar on steroids, " Michilli said.

“我们认为这个新信号可能是大型磁星或脉冲星发出的。”

A pulsar is the rapidly rotating ultra-dense remnant of a collapsed massive star.

脉冲星是一种快速转动的超高密度残骸，来自毁灭的大型恒星。

Even after a thousand years, a pulsar can still be a force to reckon with.

即使在一千年之后，脉冲星仍然是一种值得重视的力量。

The research was based on pulsar timing observations carried out with the Five-hundred-meter Aperture Spherical Telescope (FAST).

这项研究是基于500米口径球面望远镜(FAST)进行的脉冲星计时观测。

(A pulsar is the dead, ultra-dense remnant left over after a supernova.) A trickle of subsequent discoveries followed.

（脉冲星是在超新星阶段后超高密度的死亡残余。）随后小发现接踵而来。

In addition, Scott included another layer of signposts: pulsars in globular clusters orbiting the Milky Way.

此外，斯考特还查了另一层路标：绕行银河系的球状星团里的脉冲星。

These are called millisecond pulsars, and if they spun much faster the centrifugal force would rip them apart despite their tremendous gravity!

这些脉冲星被称为毫秒脉冲星，而如果它们旋转得更快，尽管它们有巨大的引力，但离心力也会将它们撕裂！