A millisecond pulsar is a supercompact neutron star, whose spin is highly accelerated by mass transferred from a companion star.
毫秒脉冲是密度极大的,转被从伴转移来的的物质大大地加快了。
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A kilonova takes place when two neutron stars or a neutron star and a black hole merge.
两颗中子或一颗中子和一个黑洞合并时,就会发生千新。
Such a star is thus known as a neutron star.
样的恒中子。
The bursts could come from neutron stars or a black hole.
爆发可能来自中子或黑洞。
Recently, we observed two neutron stars colliding.
最近,我们观测到两颗中子相撞。
But not all neutron stars disappear so quietly.
但并不所有的中子都会么安静地消失。
All neutron stars have incredibly powerful magnetic fields.
所有中子都有令人难以置信的强磁场。
The collision of two neutron stars can produce huge explosions known as kilonovas.
两颗中子的碰撞可以产生 “千新” 的巨爆炸。
Neutron stars are the remains of massive stars that have collapsed into themselves.
中子质量恒坍缩后的残骸。
The object was too massive to be a white dwarf or a neutron star.
个物体的质量太,不可能白矮或中子。
A magnetar is a neutron star with a very strong magnetic field.
磁一种具有很强磁场的中子。
Even then, the remaining neutron stars and black holes interact and fling each other way.
即便如此,剩下的中子和黑洞仍会相互作用,相互抛掷。
Neutron stars are the extremely dense remnants of supermassive stars that have exploded as supernovae.
中子极其密集的超质量体爆炸后残留下来的物体,些体曾经超新。
Many neutron stars have strong magnetic fields and as they spin, they produce radio emission.
许多中子都有很强的磁场,当它们旋转时,会发射无线电。
That is a neutron star, an image taken by the Chandra X-ray satellite.
一颗中子,些图片由钱德拉 X 射线望远镜拍摄的。
During this time, most stars are likely to die, turning into black holes or neutron stars.
在段时间里,多数恒可能会死亡,变成黑洞或中子。
On a neutron star, I'd weigh 17 trillion pounds.
而在中子上,我的体重就17万亿磅。
But they have theorized the signals could be produced by neutron stars.
但他们已经从理论上推测些信号可能由中子产生的。
Pulsars, or fast-spinning neutron stars, originate from the imploded cores of massive dying stars through supernova explosions.
脉冲,或快速旋转的中子,起源于巨的垂死恒通过超新爆炸的内爆核心。
The massive precursors to neutron stars often spin.
中子的质量前驱体经常保持自转。
The collapse of a star before it explodes in a supernova, or a very dense neutron stars colliding.
比如爆炸成超新前恒的坍缩,或高密度中子的相撞。
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