本文给出了理想流体球慢旋转结构方程的新的精确解。

This paper presented a new exact Solution for the Slow rotation Structure equation of rotating perfect fluid Spheres on neutron stars.

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不幸地，在旋转的时候，它非常的慢。

Unfortunately, it is very slow and produces some artifacts when rotating.

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接近简单的史瓦西类型(非旋转)黑洞中心的物体将会对远距离的观察者当物体接近活动视界时候存在日益增加的慢降落。

An object approaching simple Schwarzschild-type (non-rotating) black hole's center will appear to distant observers as having an increasingly slow descent as the object approaches the event horizon.

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