您要查找的是不是：
- radio supernova remnant 射电超新星遗迹
- Three Great Eyes on Kepler's Supernova Remnant. 开普勒超新星遗迹中的大三眼。
- X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant known as N63A, located in the nearby galaxy of the Large Magellanic Cloud. 来自钱德拉的X射线数据（蓝色）结合可见光（绿色）与射电（红色）数据，一道揭示了超新星遗迹N63A的新细节。N63A位于邻近星系大麦哲伦云中。
- 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。
- The supernova remnant lies about1400 light-years away towards the constellation of Cygnus. 这个超新星爆炸遗骸位于天鹅座，距离我们大约1400光年远。
- This spectacular image of the supernova remnant Cassiopeia A is the most detailed image ever made of the remains of an exploded star. 这张壮观的仙后座A照片是迄今对爆发恒星的残骸拍摄过的最精细的照片。
- Remaining at the center of the Vela Supernova Remnant is a pulsar, a star as dense as nuclear matter that completely rotates more than ten times in a single second. 船帆座超新星爆炸遗骸的中心还存在著一颗脉冲星，它是一颗如原子般致密的天体，一秒钟可以自转十次以上。
- The supernova remnant lies about 1400 light-years away towards the constellation of Cygnus. 超新星遗迹距离我们大约1,400光年远，位于天鹅座内。
- The debris then quickly thins and cools as it expands, creating a supernova remnant. 碎片随着扩散迅速变薄变冷，形成了超新星遗骸。
- In this graphic, the pulsar's position is indicated in the wider CTA 1 supernova remnant. 图中，脉冲星的位置处于CTA 1超新星残留物中。
- X-ray emission of supernova remnants. 超新星遗迹的X射线辐射。
- Although considered a "textbook" case of a supernova remnant, the intricate structure shown here reveals a few surprises. 虽然该遗迹被认为是超新星遗迹的“教科书”式样板，复杂的结构还是揭示出了几个惊人之处。
- 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。
- Today, the resulting supernova remnant has faded and is now visible only through a small telescope directed toward the constellation of Cygnus. 如今，形成的超新星遗迹已经慢慢退去，只有通过小型望远镜朝天鹅座方向看去才能看到。
- About 5 light-years long and a mere 800 light-years away, the Pencil Nebula is only a small part of the Vela supernova remnant. 铅笔星云大约有5光年长，距离我们仅仅800光年，它只是船帆超新星遗迹的一小部分。
- The complex nebula is thought to be a supernova remnant over a million years old, sprawling across the southern constellations Vela and Puppis. 这个形状复杂的星云区域分布在南天的船帆座和船尾座之间，它被认为是一个超新星残骸已经有一百万年龄。
- 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。
- Sliding your cursor over this spectacular wide field view will reveal the location of objects embedded in The Gum Nebula, including the Vela supernova remnant. 在这张壮观的广域图像上滑动你的光标，就会发现深入在甘姆星云中天体的位置，包括船帆座超新星残骸。
- By color-coding those data and combining them with Hubble's visible-light view, astronomers are presenting a more complete picture of the supernova remnant. 将其按一定的规则着色，再结合哈勃的可见光图象，天文学家呈献出的是超新星遗迹更完整的图象。
- In the only other supernova remnant (the Vela supernova remnant) where such features have been observed, the crescent shapes are clearly produced by ejecta fragments. 其他超新星遗迹中，只有一个（船帆座超新星遗迹）观测到了这样的特征，可以确信，该遗迹的新月形外观是抛出的碎片造就的。
