• They then explode, as supernovae.

    然后,它们超新星一样爆炸

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  • Smaller light echoes have been seen around supernovae.

    规模较小回音可在超新星附近看见

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  • The arrows in the top row of images point to the supernovae.

    上面一行图片中的箭头指出超新星

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  • Now this path to supernovae will have to be investigated in more detail.

    现在条产生超新星途径必须要得到更加仔细研究

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  • It comes from observations of supernovae and other very distant sources.

    而是来自遥远超新星其他非常

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  • The telescopes will also be good at spotting supernovae and gamma-ray bursts.

    这些望远镜对超新星伽马射线爆发进行定位不错

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  • Dust is produced from the winds of aging stars and from the aftermath of supernovae.

    尘埃老年恒星风暴超新星产物。

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  • By the late 1980s, a suitable standard candle had been indentified: type Ia supernovae.

    到上世纪八十年代一个合适标准烛光出现了,它就是Ia型超新星

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  • Bob Kirshner, of Harvard University, explains why supernovae are important for all of us.

    哈佛大学鲍勃·克斯勒解释了为什么超新星对我们所有人很重要

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  • The research teams raced to map the Universe by locating the most distant supernovae.

    研究队伍定位距离地球最远的超新星的办法绘制宇宙地图。

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  • Type Ia supernovae are so luminous that they outshine their host galaxies for several weeks.

    Ia超新星如此之亮以至于几个星期内它的寄主星系的光芒相形见绌。

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  • Pulsars are the dense cores left over after stars of a certain mass explode into supernovae.

    脉冲星恒星发生爆炸形成超新星遗留下来

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  • Neutron stars are, after all, a little less extreme than black holes, Big Bangs and supernovae...

    毕竟中子星没有黑洞爆炸超新星等等那么极端

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  • What both groups found was that the light from distant supernovae was fainter than predicted.

    组研究队发现遥远的超新星上发出他们预测的要微弱

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  • They were using these supernovae to measure how the universe's expansion is changing with time.

    科学家通过研究那些超新星测量宇宙膨胀随时间的变化

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  • The infrared brightness of the galaxies allowed the team to estimate how many supernovae should occur.

    星系红外亮度小组成员可以估计出超新星发生预期速率。

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  • Not just any old relics, neutron stars are the leftover cores of huge stars that exploded in supernovae.

    和一般残骸不同,中子星是以超新星方式爆炸巨大星球残余核心部分

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  • They originate from various events (supernovae and so on) within the Milky Way galaxy that is home to the Earth.

    它们可以地球所在的银河系很多事件里产生,如超新星事件

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  • Over the last 100 years, at least nine supernovae, the death explosions of massive stars, were discovered in NGC 6946.

    最近100年来至少颗超新星(质量恒星爆炸形成物)NGC6946发现

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  • "For one, the Hubble Space Telescope has weighed in on dark energy by virtue of the measurements of supernovae," he said.

    “例如,超新星测量方面具有优势哈勃太空望远镜被用于能量项目,”

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  • Examining as many supernovae as possible can help researchers measure how fast galaxies are moving away from one another.

    尽可能地检测超新星能够帮助研究人员测量星系之间的背离速度。

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  • Unlike most supernovae, this one spewed lots of elements far heavier than iron, including radioactive thorium and uranium.

    颗晕星不同于大多数超新星它吐出许多元素其中包括放射性

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  • Researchers first observed accelerated expansion by studying Type Ia supernovae-the explosive deaths of White Dwarf stars.

    研究人员研究Ia型超新星——白矮星爆炸中的消亡过程时首度观察到加速膨胀

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  • IceCube's task is to watch for energetic neutrinos emanating from violent cosmic events such as supernovae and gamma-ray bursts.

    冰立方任务找到那些一些剧烈宇宙事件超新星伽马射线爆发中发射不来的高能中微子。

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  • Supernovae of this type have been observed for decades and we have learned that they are very predictable in the way they evolve.

    这种超新星已经观测了好多年我们知道它们能够按照它们的演变规律可以预测的。

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  • The supernovae make the chemical elements through real alchemy, transforming one element, the light elements into the heavy ones.

    超新星通过真正点金术制造化学元素,把一种元素元素转变成的。

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  • There are a number of kinds of stellar explosions that can produce supernovae — which are short-lived, extra bright stellar events.

    一些不同种类恒星爆炸可以产生超新星——短时间的,异常明亮的恒星爆炸事件

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  • One particular sort, though, known as type Ia supernovae, always explode with about the same energy and are therefore equally bright.

    不过,有一类称为Ia型的超新星爆炸时释放的能量始终基本相同因此量度也相同。

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  • Supernovae studies have allowed scientists to see that dark energy has been impacting galaxies since as far back as nine billion years ago.

    有关超新星研究使科学家了解到,追溯到90亿能量已经开始影响星系

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  • Supernovae studies have allowed scientists to see that dark energy has been impacting galaxies since as far back as nine billion years ago.

    有关超新星研究使科学家了解到,追溯到90亿能量已经开始影响星系

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