超新星爆发

行星躲过超新星爆发的几率总是十分渺茫。

The chances of a planet surviving a supernova always looked terribly slim .

坍缩阶段中微子对II型超新星爆发的影响

How the Neutrino in Collapse Phase Affect Type ⅱ Supernova Explosion

10M⊙的超新星爆发。

10M_ ⊙ of a supernova .

RM不稳定性在天体物理中的超新星爆发过程以及惯性约束核聚变中，都扮演着重要的角色。

The RM instability plays an important role in applications ranging from the supernova in astrophysics to combustion in inertial confinement fusion ( ICF ) .

这类名为Ia型的超新星爆发由于可以在很远的距离上被观测到，并且亮度遵循可靠的模式，它们被当成测量宇宙膨胀的里程计。

These supernovae , called Type1a , serve as cosmic mile markers to measure expansion of the universe because they can be seen at large distances , and they follow a reliable pattern of brightness .

综述了Ⅱ型超新星爆发过程中涉及到的物理因素和数值计算方法，例如电子俘获，物态方程，差分格式以及GR流体动力学方法。

Besides , we summarized physical factors and numerical calculation method in type ⅱ supernova , such as electronic captured and the equation of state , array of difference and the general relativity hydrodynamic method .

讨论了迄今超新星爆发理论中各种爆炸性核燃烧核合成26Al的问题。

Nucleosynthesis of ~ 26Al in explosive nuclear burning of supernovae is discussed .

恒星在超新星爆发后又如何呢？

What will happen to the remains of the supernova explosion ?

综述了与超新星爆发机制研究中的相关理论研究进展。

The research progress relevant to explosion mechanism is summarized .

这种情况发生的一种可能是由于附近的超新星爆发；

One way this may happen is if a supernova explodes nearby .

Ⅱ型超新星爆发物理机制的研究概况

A Survey of Studies on the Mechanism of Type ⅱ Supernova Explosions

Ⅱ型超新星爆发的中微子过程

The neutrino processes in the explosion of type ⅱ supernovae

成团超新星爆发的热自模解

Self-similar Solution of Thermal Conduction during Collective SN Explosions

利用超新星爆发测量电子中微子静止质量

Measurement of electron neutrino mass by supernova neutrino bursts

在超新星爆发的复杂动力学中，电子俘获起着关键的作用。

Electron capture plays a pivotal role in the complex dynamics of supernova explosion .

超新星爆发是非常复杂的事件。

Supernova explosions are immensely complicated events .

通过放射性碳研究超新星爆发事件

A study of supernova explosion with radiocarbon

恒星演化和超新星爆发理论中某些重要问题的核物理问题

Some important questions of nuclear physics on the theoryof both stellar evolution and supernova explosion

超新星爆发发射的γ射线的能量

The Gamma-ray Energy Output from Supernova Explosion

超新星爆发的前身星模型研究

Studies of Progenitor Models for Supernova Explosion

超新星爆发会瓦解双星系统。

The supernova explosion disrupts the binary .

本文解析地讨论了能量从持续点状源向外热传播的自模问题，得到成团超新星爆发的热自模解。

We discuss explicitly the self-similar solution of thermal conduction from a point-like steady source .

有些恒星在壮观的超新星爆发中消亡，遗留下这样的残余。

And some stars die spectacularly in a supernova explosion , leaving remnants like that .

Ia型超新星爆发理论（Ⅱ）：理论研究中的重要疑难问题

On Explosion Theory of Supernova Type I_a ( II ): Important Unsolved Problems in Theoretical Study

这对恒星晚期演化和超新星爆发研究可能会有重要的影响。

The screening effect may importantly influences the study of stellar late stage evolution and supernova burst .

尽管如此，对其他同位素的观察表明，太阳系星云形成时确有一次超新星爆发。

Nevertheless , other isotopes suggest a supernova did go off just as the solar nebula was forming .

讨论了在以冷暗物质为主的宇宙中，超新星爆发对矮星系演化的反馈作用。

The feedback effect of supernova explosions on dwarf galaxies in the cold dark matter dominated universe is studied .

作为应用，本文分析了矮星系并合形成大星系这一模型中成团超新星爆发时能量传播的各个阶段。

As an application , we analyze the energy propagation during collective SN explosions in a merging model of galaxy formation .

当超新星爆发时，可以存在一个以纯热传导为主的能量传播阶段。

When supernovae explode , there may exist a period when pure thermal conduction is the dominant process of energy propagation .

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。这时如果地球和月亮的中心大致在同一条直线上，月亮就会进入地球的本影，而产生月全食。

The bright source at the center of the image is presumed to be a neutron star created during the supernova .