超新星

在我们的星系中每10年至少有一颗超新星出现。

At least one supernova occurs per decade in our galaxy .

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 .

有些超新星研究者怀疑，这可能只是昙花一现。

Some supernova researchers wondered if it might be just a nine-day wonder .

十多年以来，天文学家们一直在猜想，超新星激波可以充当巨型粒子加速器。

Astronomers have suspected for more than a decade that supernova shock waves can act like giant particle accelerators .

他们认为这个庞大的物体是由两颗“白矮星”合并而成的，通常白矮星会以强大的超新星的形式爆炸。这颗新星被天文学家称为“白矮星”。

The new star is what astronomers1 call a ' white dwarf2 ' .

II型超新星的物态方程与爆发能量

The Equation of State and Explosive Energy of Type II Supernova

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

超新星有两类：I型和II型。

There are two main classes , Type I and Type II .

II型超新星瞬发爆炸模型的激波传播

C shape ; Shock Propagation in the Prompt Explosion Model of SN II

研究了这19个伴有OH1720MHz脉泽发射的混合形态超新星遗迹的X射线特征。

The X-ray characteristics have been studied .

超新星在星际~（26）Al问题中的作用：星际~（26）Al的天体源泉问题之三

The Origin of the Interstellar ~ ( 26 ) Al (ⅲ): The Role of Supernovae

另外，我们的光谱拟合可以为C＋O星作为Ic型超新星的前身星提供证据。

The modeling may provide evidence for C + O stars as progenitors of Type Ic supernovae .

用MonteCarlo方法拟合超新星SN1993J的早期光谱

Modeling the Early Spectra of SN 1993J Using the Monte Carlo Method

这个模型的重要点是从超新星遗迹来的X射线促使产生OH分子。

An important ingredient of this model is that X-ray emission from the remnant enhances the production of OH molecules .

超新星爆炸时发射出大量的无线电射线、X射线和宇宙射线以及其他粒子。

Supernova explosions release tremendous amounts of radio radiation , x-radiation and cosmic rays , as well as other elements .

由物质吸积导致的Ia型超新星会在爆发前产生大量的X射线辐射。

A Type1a supernova caused by accreting material produces significant X-ray emission prior to the explosion .

最后，我们还探讨了Ia超新星中碳点火的非线性问题。

Finally , nonlinear process of carbon ignition is discussed .

不透明度对Ia超新星极大光度的影响

Effect of Opacity on the Maximum Absolute Bolometric Magnitude of Ia Supernova

对Ib／Ic型超新星应加以特别关注。

Particular attention should be paid to the sample of Type Ib / Ic SNe .

Ia型超新星的爆发机制及其前身星模型

The Explosion Models and Progenitors of Type la Supernovae

旋涡星系中Ia超新星的产生率比椭圆星系的要高。

Spirals are more efficient SNe Ia producers , comparing with elliptical galaxies .

研究队伍用一种Ia型超新星做研究。

The teams used a particular kind of supernova , called type Ia supernova .

相反，来自双白矮星并合的超新星产生的X射线辐射要比吸积少很多。

A supernova from a merger of two white dwarfs , on the other hand , would create significantly less X-ray emission than the accretion scenario .

接着又发生两起爆炸现象，宇航员总结道：最终SN2009ip还是变成了超新星。

Following two subsequent flare-ups , astronomers have now concluded that SN 2009ip has gone supernova at last .

其中一种称为ia型的超新星发出的能量几乎完全一样。

Some , called type Ia , always explode with almost exactly the same energy .

Ia超新星在宇宙学中的应用

Application of Type Ia Supernovae to Cosmology

超细粉的电爆法制备及其设备的开发II型超新星的物态方程与爆发能量

Preparation of Metallic Ultra-fine Powders Using Wire Electrical Explosion Method and Development of the Apparatus ; The Equation of State and Explosive Energy of Type II Supernova

金刚石携带分别由p过程和r过程产生的Xe同位素组分（XeHL），其源区可能是超新星。

Diamond contains Xe isotopes ( Xe HL ) typically produced in p and r processes , probably formed in supernovae .

10M⊙的超新星爆发。

10M_ ⊙ of a supernova .

你见过超新星的照片么？【我没见过supernova我对mininova很熟……囧】

Have you ever seen picture of a supernova ?