supernova star

It first drew attention in 2009, when it flared up brightly in an apparent supernova-a star exploding at the end of its life.

在2009年它首次引起人们注意，当时它骤然爆炸成为一颗超新星，并发出闪耀的光芒。超新星就是恒星在演化末期时经历的一种剧烈爆炸。

The supernova was precipitated when the core of massive star imploded to form a star.

超新星的形成是当大质量恒星核心爆裂时产生中子星的时候.

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.

They studied a once-massive star that went supernova about 100000 years ago.

他们研究了一颗近10万年前发生超新星的恒星，这颗恒星在消亡前质量很大。

The new modeling finds that a supernova, or exploding star, could indeed have triggered birth of our sun in a dense cloud of gas and dust, the researchers say.

研究人员称，最近的这次模拟发现，一颗超新星（爆炸中的恒星）的确有可能导致太阳在一团浓密的气体与尘埃中诞生。

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。

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。

The EOS of asymmetric nuclear matter is crucial for understanding many astrophysical problems and phenomena related to the global properties of neutron stars, supernova explosion and neutron star cooling.

非对称核物质的状态方程在理解中子星的整体性质，超新星的爆发、中子星的冷却等许多天体物理的现象中起着决定性的作用。

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。

1054-A supernova is observed by the Chinese and Amerindians near the star Tauri.

1054年的今天，一颗位于金牛座附近的超新星被中国及印第安人发现并记载。