脉冲星

There may be a real physical cause for dispersion of the pulsars out of the plane.

银道面外脉冲星数的弥散也许有其真正的物理原因.

The 3 P 2-superfluid phase transition model for pulsar glitches.

脉冲星周期突变的3P2中子超流涡旋涡旋相振荡模型.

An introduction on the definition of binary pulsar time BPT was given.

对由双星系统内毫秒脉冲星的轨道运动定义的双星脉冲星时也做了介绍.

A pulsar is a celestial object that emits light in short burst.

脉冲星是一种能够发出光脉冲的天体.

Each pulsar or neutron star is the fast-rotating, dead heart of a once-massive star.

每一颗脉冲星或中子星都曾是大质量恒星死后快速旋转的核心.

But certain stars, called pulsars , give off regular pulses of radio waves.

但有些恒星, 所谓的脉冲星, 会有规律地发出射电波脉冲.

The perspective of the pulsar observation of the FAST program is outlined.

展望了FAST望远镜观测脉冲星的前景.

They have discovered now , previou sly unimagined objects-pulsars, quasars, and black holes.

他们发现了以往想象不到的新客体 —— 脉冲星 、 类星体和黑洞.

Interest was renewed in the astronomical community with the discovery of pulsars.

天文学团体随着脉冲星的发现重新激发了兴趣.

They have discovered now, previously unimagined objects-pulsars, quasars, and black holes.

他们发现了以往想象不到的新客体 ― ―脉冲星 、 类星体和黑洞.

Another kind of period variation, " Glitches, " are seen in several pulsars.

在几个脉冲星中还看到了周期的另一种变化, 即 “ 自转突快 ” 现象.

First of all the reason of the pulsar dispersion and several popular de-dispersion algrithms are introduced.

首先介绍了脉冲星的色散形成原因以及几种当今流行的消色散算法.

Structure of a pulsar — a rotating magnetic neutron star.

脉冲星的结构.一颗旋转磁中子星.

Some pulsars keep time better than the earth's most accurate clocks.

某些脉冲星发送脉冲比地球上最精确的时钟都准时。

Pulsar : A dense, rapidly rotating star that emits pulses of light.

脉冲星: 高密度 、 快速旋转、发射脉冲光的星体.