1.
The supernova explosion disrupts the binary.
超新星爆发会瓦解双星系统。
2.
Supernova explosions are immensely complicated events.
超新星爆发是非常复杂的事件。
3.
How the Neutrino in Collapse Phase Affect Type Ⅱ Supernova Explosion
坍缩阶段中微子对II型超新星爆发的影响
4.
In fact, the cosmic Crab is now known to be a supernova remnant, an expanding cloud of debris from the death explosion of a massive star.
实际上,现在我们知道蟹状星云是超新星爆发的遗迹,即一个巨大恒星死亡后爆炸的残屑云。
5.
The bright source at the center of the image is presumed to be a neutron star created during the supernova.
图片中心的明亮辐射源据信是超新星爆发过程中产生的中子星。
6.
One way this may happen is if a supernova explodes nearby.
这种情况发生的一种可能是由于附近的超新星爆发；
7.
Theory predicts that a star with a mass between eight and25 times that of our sun ends its life in a supernova explosion.
当一颗恒星的质量介于太阳质量的8~5倍时，理论预测它将会以超新星爆发的形式结束生命。
8.
There is a good chance that this outward diffusion of neutrinos and antineutrinos plays a crucial role in the supernova explosion.
中微子和反中微子的这种向外的散射很可能在超新星爆发中起着关键的作用。
9.
Physical Explanation to SU UMa-type Dwarf Nova s Explosion and Super-explosion;
SU UMa-type矮新星爆发和超爆发的物理解释
10.
The Equation of State and Explosive Energy of Type II Supernova
II型超新星的物态方程与爆发能量
11.
The hot gas will be heated further by any supernova which go off in the galaxy.
热气体将被星系中爆发的任何超新星进一步加热。
12.
In theory, the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova.
理论上，形成一颗毫秒脉冲星的第一步，是一个大质量恒星在成为超新星而爆发后留下的中子星。
13.
Supernova remnants: What is left after a heavy star violently explodes.
超新星遗迹：超重星体爆炸后所剩下的残迹。
14.
NASA's Hubble Sees Brightest Supernova Explode Ever?
还有比超新星爆炸重要的新闻吗？
15.
The farther away the supernovae are, the longer their light has been traveling and the further back in time the explosion occurred.
超新星越远，它们的光旅行的距离越长，爆炸发生的时间就越古老。
16.
Research on the Physical Process and Explosion Mechanism of Core-collapse Supernova;
核心坍缩型超新星的相关物理过程及爆发机制的研究
17.
The supernovae exploded between3.5 and10 billion years ago.
超新星爆炸时间在35-100亿年前。
18.
Positron Capture on ~(55)Co at Presupernova and Supernova Conditions;
超新星爆前天体和超新星条件下~(55)Co的正电子俘获