查询词典 neutron star

"Just after it was born, this neutron star got a one-way ticket out of the Galaxy," said co-author Robert Petre of NASA's Goddard Space Flight Center in Greenbelt, Md."Astronomers have seen other stars being flung out of the Milky Way, but few as fast as this."

"就在刚出生后不久，这个中子星就得到了一张离开银河系的路票"来自NASA的Goddard宇宙发射中心的共著者 Robert Petre 说到"天文学家已经观测到其他恒星冲出银河系，但很少有他这么快的"

The breakneck speed of the Puppis A neutron star, plus an apparent lack of pulsations from it, is not easily explained by even the most sophisticated supernova explosion models.

"这个宇宙泡状球体的难迷惑就在于在自然条件下是如何弄出这么强有力的大炮"Winkler说到。高速可以被解释成由常见的高能量爆炸引起，但是模型非常复杂并很难适用于真正的爆炸。

It is a neutron star spinning just under 100 times per second and emitting regular radio pulses like a lighthouse beam.

这是一颗每秒钟自转接近100次的中子星，它象灯塔光束一样发射出规则的射电脉冲。

The radio pulses from the neutron star were no longer regular. Astounded, he noted the pattern of the pulses as they came in now.

当这个人朝着通话信道大叫时，天文台的其他人还以为他不过是像一个小男孩弄丢了游戏中的弹子

In each case, the neutron star is orbiting within the outer atmosphere of its supergiant companion.

无一例外，中子星的轨道都在其巨星同伴的外层大气之中。

Now, Lorimer says, the evolutionary connections between the two are strengthening, and observations like this one will help "elucidate our understanding of what happens to a young neutron star after its birth in a supernova."

现在，这两者之间表现出了强有力的进化联系。这类发现可以帮助我们弄清楚当一颗新的中子星从超新星中诞生后还会发生些什么。

The influences of hyperon coupling constant on the properties of neutron star were studied by making use of -GL85 parameter set in the framework of the relativistic mean field theory and taking, freedoms of hyperons into consideration.

采用相对论平均场理论下的GL85参数组，在考虑超子Λ，Σ(上标+，Σ^0，Σ，Ξ^0，Ξ自由度下，研究超子耦合常数的选取对中子星内粒子数密度分布、状态方程及质量－半径关系的影响。

The various effective interactions'(including DDME1,TW99,NL2,TM1,TM2,GL85 and GL97) influence on the constitute, equation of state and mass of neutron star are studied in the framework of relativistic mean field theory considering the interacting nucleons, hyperons and mesons system at finite temperature (T=20 MeV).

从相对论平均场（Relativistic Mean Field，RMF）理论出发，考虑核子、超子和介子的相互作用，研究了一定温度（T=20 MeV）下，各种不同相互作用参数组（DDME1、TW99、NL2、TM1、TM2、GL85和GL97）对中子星物质的粒子组成、状态方程和质量等的影响。

In the theoretical framework of the relativistic mean field, the influences of π- meson condensate on the equation of state and the particle fractions of neutron star matter including delta isobars are studied.

在相对论平均场理论框架下研究了π-介子凝聚对包括Δ共振态的中子星物质状态方程及其粒子分布的影响。

"Just after it was born, this neutron star got a one-way ticket out of the Galaxy," said co-author Robert Petre of NASA's Goddard Space Flight Center in Greenbelt, Md."Astronomers have seen other stars being flung out of the Milky Way, but few as fast as this."

&就在刚出生后不久，这个中子星就得到了一张离开银河系的路票&来自NASA的Goddard宇宙发射中心的共著者 Robert Petre 说到&天文学家已经观测到其他恒星冲出银河系，但很少有他这么快的&

Neither the killing of Mr Zarqawi nor any breakthrough on the political front will stop the insurgency and the fratricidal murders in their tracks.

在对危险的南部地区访问时，他斥责什叶派民兵领导人对中央集权的挑衅行为。

In fact,I've got him on the satellite mobile right now.

实际上 我们已接通卫星可视电话了