white dwarf

It is then referred to as a White Dwarf .

这时，它被称为白矮星。

Discovery of X-ray Selected AGNs , a White Dwarf and a Cataclysmic Variable

新发现的X射线选活动星系核、白矮星和激变变星

A Practical Negative-Energy Spectrum System & The White Dwarf Star

一个实际存在的负能谱系统&白矮星

Then the white dwarf will collapse and becomes a neutron star .

变成个中子星，当我们测量中子星的。

Analysis of Quanta Statistic Theory on White Dwarf

量子统计理论对白矮星的分析

The researchers suggest that there are many white dwarf stars throughout this halo .

研究人员猜想，光晕内到处有白矮星。

The Upper-limit of the Equilibrium Mass of the White Dwarf Star

白矮星的平衡质量上限

It may be the remains of a carbon-rich white dwarf star .

它很可能是白矮星留下的残余物，白矮星核心堆积有大量的碳。

The fundamental properties of white dwarf star in the evolution process of early stage has been analysed in detail .

详细地剖析了初期演化过程中的白矮星的基本特性。

The picture on the left shows a White Dwarf and the one on the right shows a Supernova .

左边的图片就是白矮星，右边的是超新星。

This implies that white dwarf mergers dominate in these galaxies .

这意味着，白矮星并合是这些星系中的主导过程。

Or , it seems , when you 're cruising past a white dwarf star .

或者可以说在你缓慢驶过一颗白矮星时。

The nova phenomenon generally occurs in a binary system that has as one member a very hot white dwarf .

新星这种现象一般发生在双星系统中，其中一颗子星是非常热的白矮星。

It will quietly and steadily burn the hydrogen to helium and become a white dwarf .

它会稳定地把氢转化为氦，然后安静的死去，成为白矮星。

His team used observations from NASA 's Spitzer space telescope to investigate dead white dwarf stars .

他的队伍通过美国国家航空与宇宙航行局的施皮策望远镜去观察一些白矮星。

I 've found that these three questions can help determine whether a secret is a white dwarf or a black hole .

我发现下面3个问题能够帮助断定一个秘密是白矮星还是黑洞。

When a star collapses , it can become either a White Dwarf or a Supernova .

当恒星塌陷时，可以成白矮星，也可以是超新星。

When a star collapses , it will be White dwarf or Supernova .

当恒星塌陷时，它会变成白矮星或者超新星。

" A white dwarf is like a smoking cinder from a burnt-out fire ," Williams said .

白矮星就像是火焰已熄、但还冒着烟的煤渣。

If a star is small , it collapses and remains collapsed , this is called a White Dwarf .

如果是小的，塌陷时就会留在塌缩状态，这就是白矮星。

In other words , the white dwarf acts like a lens that makes the bigger star appear brighter during the eclipse .

换句话说，白矮星充当了透射镜片的作用，使得在日月食现象时较大的恒星候变得更加明亮。

Badenes 's team examined archival observations and found a white dwarf and neutron star orbiting one another extremely closely .

Badenes的团队试验档案观测并发现白色小的中子星体非常近的围绕另一个运转。

As the white dwarf spins , the columns of infalling gas rotate with it .

当白矮星自转时，被吸入的气柱也跟著一起转起来。

The tightly wound white dwarf binary should also be radiating gravitational waves - ripples in the fabric of space and time .

紧紧缠绕的白矮双子星同时也会发出引力波——那是在空间和时间结构上扩散开的波纹。

The observations also show for the first time that a white dwarf can create a cavity around it before blowing up in a Type Ia event .

观测结果还首次显示，白矮星在爆炸成为Ia型超新星之前，会在其周围创造一个空洞。

Since a 7-solar-mass is too large to be a white dwarf or neutron star , it must be a black hole .

因为有着7个太阳质量的星体不可能是白矮星或中于星，所以它一定是黑洞。

An open question remains whether these white dwarf mergers are the primary catalyst for Type1a supernovae in spiral galaxies .

剩下的开放问题是，在旋涡星系中，这些并合的白矮星是否就是Ia型超新星的主要催化剂。

The White Dwarf Star Sytems & The Composite System Compased of the Electron-Positive Energy System and the Helium-Ion-Negative Energy System

白矮星系统&正能谱电子系统与负能谱氦离子系统的复合系统

This article employ the new theory ( PNES thermodynamics theory ) in the point of view of the composite system to study the mechanical equilibrium of white dwarf stars .

本文应用这一新理论（PNES热力学理论），以复合系统的观点研究了白矮的力学平衡问题。

After this point , it would collapse into something like a sputtering white dwarf or neutron star , and then-if its mass kept increasing-eventually become a black hole .

自那以后，它会不断坍缩，直到变成一颗白矮星或者中子星——如果质量还是不停增加，它最终会变成一个黑洞。