white dwarf star

Most scientists agree a Type1a supernova occurs when a white dwarf star a collapsed remnant of an elderly star exceeds its weight limit, becomes unstable and explodes.

大多数科学家认为，当白矮星（年老恒星坍缩而成的残骸）超过质量极限，变得不稳定并爆发的时候，会产生Ia型超新星。

互联网摘选

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。

互联网摘选

The sun's upper layers will expand and lose material, and eventually the core will cool enough to become a white dwarf star, and finally a black dwarf.

太阳的上层也将扩大，失去物质重量，最后中心冷却到一定程度就成了白矮星，最终成黑矮星。

互联网摘选

Obviously, that the original theory can't reflects the practical state of white dwarf stars, because the white dwarf star ( isn't) a electron system but a composite system which is composed of the electron sub-system and helium-ion sub-system.

显然原有理论不能反映白矮星的实际状态，因为白矮星并不是一个电子系统而是一个由电子子系和氦离子子系组成的复合系统。

互联网摘选

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。

互联网摘选

The evolution of fixed star having something to do with nuclear reaction, the star generally loses partial mass in its final period and finally collapses into compact star ( white dwarf, neutron star or black hole).

恒星的演化与核反应有关，演化到晚期的恒星一般要损失一部分质量，然后坍缩成致密星（白矮星、中子星或黑洞）。

互联网摘选

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

互联网摘选

How such a dense planet formed is unclear, the researchers say, but it's probably the crystalline vestige of a white dwarf star whose atmosphere was stripped away by the parent pulsar.

研究人员称，至于密度这么高的行星是如何形成的，这一点尚不清楚，但它很可能是一颗被主脉冲星剥夺了大气的白矮星留下的晶体残骸。

互联网摘选

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

互联网摘选

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。

互联网摘选

Who they are: Ray Palmer is a physicist who, will studying the molecular density of a white dwarf star, gains the ability to reduce his molecular density.

他们是谁？雷·帕尔默是一名科学家，后通过研究一块白矮星碎片获得了压缩自身分子结构的能力。

互联网摘选

Theory predicts that a white dwarf star will explode when infalling matter from a companion star increases the mass of the white dwarf beyond a critical mass limit, known as the Chandrasekhar limit.

理论预言，当来自伴星的物质让白矮星的质量增加到了临界质量极限即钱德拉塞卡极限时，白矮星就会爆发。

互联网摘选

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。

互联网摘选

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。

互联网摘选

According as the original theory has regarded the white dwarf star system is a electron system alone, the helium-ion system is only looked as a external condition that the electron system is restricted.

但是PNES理论的基本原理和思路与原有的理论完全不同，按照原有理论，白矮星系统只是一种电子系统，氦离子系统只被视为约束电子系统的外部约束条件。

互联网摘选

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

白矮星的平衡质量上限

互联网摘选

The white dwarf star at the center of this planetary nebula may be accompanied by a second-generation world, formed from the debris of the dying star's original planets.

这颗濒临死亡的恒星将原有行星撕成碎块，第二代行星形成于这些碎块。

互联网摘选

Applying the new theory-the positive and negative energy spectrum ( PNES) thermodynamical theory to the mechanical equilibrium of white dwarf stars, the mechanical equilibrium of white dwarf star at early stage has been analysed carefully.

将一个新理论&正、负能谱（PNES）热力学理论应用于白矮星系统的力学平衡问题，对白矮星初期演化阶段的力学平衡进行了详细的分析。

互联网摘选

Another hypothesis is that the unusual radio source originates from a binary system containing a hot white dwarf, neutron star, or black hole, and that the waterfall is just a jet from this energetic system.

另一个假说认则为这种不寻常的射电源源于二进制系统，包含热白矮星、中子星或黑洞，瀑布只是能量系统在释放而已。

互联网摘选

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。

互联网摘选

The collapse of a star may produce a White Dwarf or a neutron star& a star, whose matter is so dense that it continually shrinks by the force of its own gravity.

一颗超新星的崩溃可能会产生白矮星或中子星，其物资的密度非常大以至于在其自身重力的作用下持续收缩。

互联网摘选

After it swallows the Earth, it will instead go through some phases of expansion and collapse, and will eventually settle down, leaving behind a small white dwarf star with the bullet still lodged in the center.

在它吞没地球后，它会经历一系列的膨胀和坍缩，最终一切都安宁下来，只留下一颗小小的白矮星，而那颗子弹还留在中央。

互联网摘选

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。

互联网摘选