Three great eyes on Kepler's supernova remnant.
开普勒超新星遗迹中的大三眼。
This image shows a part of the circular supernova remnant known as RCW 86.
这张照片显示的是环形超新星残骸的一部分，名叫RCW86。
Oddly, the star was significantly displaced from the center of the supernova remnant.
更怪的是，这颗星体的位置明显地偏离 超新星残骸的中心。
This shock wave sweeps up an expanding shell of gas and dust called a supernova remnant.
这种激波会导致形成一个膨胀的气体和尘埃构成的壳状结构，这被称作超新星遗迹。
The supernova remnant is within the plane of our Milky way Galaxy and is 2,600 light-years away.
超新星的残骸位于银河系的平面内，距离地球2600光年。
This supernova remnant is unusual in that its X-ray emissions are largely non-thermal in origin.
这一超新星残体的不寻常之处是，其x -射线发射基本上不是热源的。
Can you find, in the above image, a comet, a spiral galaxy, an open star cluster, and a supernova remnant?
在上面图中，你能找到：一彗星，一旋涡星系，一疏散星团和一超新星遗迹吗？
The nebula is a large supernova remnant, an expanding cloud born of the death explosion of a massive star.
该星云是超新星的遗迹，是一个大质量的恒星死亡爆炸时的扩散云气形成的。
This 1991 image from NASA's Hubble Space Telescope captures a small section of the Cygnus Loop supernova remnant.
这幅由哈勃空间望远镜摄于1991年的图像捕捉到了天鹅座Loop超新星的一小段残骸。
The Veil Nebula itself is a large supernova remnant, the expanding debris cloud from the death explosion of a massive star.
面纱星云本身是一个巨大的超新星遗迹，这是巨恒星濒死时爆炸产生的残骸云体，正在不断扩张。
The cycle of life brings even huge stars to dust, as highlighted by a newly released picture of the supernova remnant G54.1 0.3.
再巨大的星辰也逃不过生命的循环，终有一日会变为尘埃，公布于2010年3月29日照片中的超新星残骸g54.1.0.3非常好的说明了这一现象。
However, if the supernova remnant exceeds three solar masses, conventional physics suggests a black hole should be left behind.
然而，如果超新星的残核大于三个太阳质量，按常规物理法则来说，就将成为黑洞。
When the Hubble Space Telescope was pointed at the supernova remnant in 1994, however, the existence of curious rings was confirmed.
1994年，哈伯太空望远镜为这个超新星遗骸拍摄了一系列照片，确认了这些奇特环状结构的存在。
Identified as E0102-72, the supernova remnant lies about 190,000 light-years away in our neighboring galaxy, the Small Magellanic Cloud.
名为e0102- 72的超新星遗骸，位在邻近的小麦哲伦星系内，离我们约有190,000光年远。
We list a sample of 50 pairs of pulsar (PSR) and supernova remnant (SNR) associations which have been suggested from over 230 SNRs and 1300 PSRs.
从所有已被提出和发现的230多颗超新星遗迹和1300多颗脉冲星中，总结出一个共50对脉冲星与超新星遗迹成协候选体的样本。
In fact, the cosmic jellyfish is seen to be part of bubble-shaped supernova remnant IC 443, the expanding debris cloud from a massive star that exploded.
这个宇宙级水母被看作是泡泡状的超新星遗迹IC 443的一部分。 超新星遗迹是大质量恒星爆发时向外扩张的碎片云。
Because the distance to the supernova remnant is about 7,000 light-years, that explosion actually happened 7,000 years before the light reached Earth in 1006.
因为超新星遗迹距离我们大约7,000光年远，所以在1006年到达地球的光实际上是由7,000年前发生的爆炸发出的。
This image provided by NASA combines infrared images from the ground (red, green) with X-Ray data from NASA's Chandra X-Ray Observatory in the supernova remnant W49B.
由美国宇航局提供。这张图像结合了来自地面(红色、绿色)的红外图像和来自钱德拉X射线天文台超新星残骸W49B的X射线数据。
"This supernova remnant got really big, really fast," says Brian J. Williams, a postdoctoral research scholar at North Carolina State University, where researchers led a team of astrophysicists.
“这个超行星遗迹成长得非常大、非常快，”来自北卡罗来纳州立大学(许多研究学者在此地成立了天体物理学家团队)的博士后研究学者-布莱恩·j·威廉姆斯说。
It is the remnant of a supernova that was recorded by Chinese and Arab astronomers in 1054.
早在1054年，中国和阿拉伯天文学家就有关于它是超新星残余的记载。
A 30-year-old object believed to be the youngest black hole ever seen, is a remnant of SN 1979c, a supernova in the galaxy M100, shown here, approximately 50 million light-years from Earth.
一个三十岁年龄的天体据信是人类观察到的最年轻的黑洞，它是M 100星系里名为SN 1979c的超新星的余烬，距离地球大约5000万光年，如上图所示。
Now the galaxy is full of gas and dust, which could hide a distant supernova optically, but the remnant would still produce detectable radio waves and X-rays.
现在，星系充满了气体和灰尘，掩盖了遥远的超新星的可见性，但是(它的)残骸依然放射出可检测的无线电波和X射线。
A pulsar is not a normal star, but a dense, rapidly spinning remnant of a supernova explosion.
脉冲星并不是一种正常的恒星，它是超新星爆炸后留下的高密度快速旋转的残余部分。
Immediately after supernova, if the remnant core has a mass of less than three SUNS, one would expect a blob of degenerate neutron matter to be spinning in the explosion's wake.
在经历超新星后，假如剩下的残核小于三个太阳质量，爆炸的残余物质就将可能演变成旋转着的中子团。
It is the remnant of a supernova explosion in the year 1054 much more about that during my next lecture and what you see here is not stuff that is generated at this moment in time by the pulsar.
它是超行星在1054年，爆炸后的剩余物4，下节课我会，详细讲它，这里你看到的不是，脉冲星那时，聚集的物质。
It is the remnant of a supernova explosion in the year 1054 much more about that during my next lecture and what you see here is not stuff that is generated at this moment in time by the pulsar.
它是超行星在1054年，爆炸后的剩余物4，下节课我会，详细讲它，这里你看到的不是，脉冲星那时，聚集的物质。
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