On a neutron star, I'd weigh 17 trillion pounds.

而在中子星上，我的体重就17万亿磅。

Such a star is thus known as a neutron star.

这样的恒星被称为中子星。

The bursts could come from neutron stars or a black hole.

爆发可来自中子星或黑。

Recently, we observed two neutron stars colliding.

最近，我们观测到两颗中子星相撞。

He also did groundbreaking work on neutron stars and black holes.

他还在中子星和黑方面进行了开创性的研究。

But not all neutron stars disappear so quietly.

但并不所有的中子星都会这么安静地消失。

But they have theorized the signals could be produced by neutron stars.

但他们已经从理论上推测这些信号可中子星产生的。

Short ones are from merging neutron stars.

短的则来自合并的中子星。

The collision of two neutron stars can produce huge explosions known as kilonovas.

两颗中子星的碰撞可以产生被称为 “千新星” 的巨大爆炸。

Neutron stars are the remains of massive stars that have collapsed into themselves.

中子星大质量恒星坍缩后的残骸。

That is a neutron star, an image taken by the Chandra X-ray satellite.

这一颗中子星，这些图片钱德拉 X 射线望远镜拍摄的。

The object was too massive to be a white dwarf or a neutron star.

这个物体的质量太大，不可白矮星或中子星。

A kilonova takes place when two neutron stars or a neutron star and a black hole merge.

两颗中子星或一颗中子星和一个黑合并时，就会发生千新星。

Neutron stars are the extremely dense remnants of supermassive stars that have exploded as supernovae.

中子星极其密集的大质量星体爆炸后残留下来的物体，这些星体曾经新星。

A freshly minted neutron star might spin several times per SECOND.

一颗新造的中子星可每秒就会旋转几次。

We don't know of any about-to-merge neutron stars, either.

我们也不知道任何即将合并的中子星。

Many neutron stars have strong magnetic fields and as they spin, they produce radio emission.

许多中子星都有很强的磁场，当它们旋转时，会发射无线电。

The same is true for the star's core when it collapses into a neutron star.

当恒星的核心坍缩成中子星时，情况也如此。

All neutron stars have incredibly powerful magnetic fields.

所有中子星都有令人难以置信的强大磁场。

Even then, the remaining neutron stars and black holes interact and fling each other way.

即便如此，剩下的中子星和黑仍会相互作用，相互抛掷。