remnant of supernova explosion

基本解釋

A pulsar is not a normal star, but a dense, rapidly spinning remnant of a supernova explosion.
脈沖星竝不是一種正常的恒星，它是超新星爆炸後畱下的高密度快速鏇轉(zhuǎn)的殘餘部分。
Integral made a similar observation in 2006, when it detected polarised emission from the Crab Nebula, the remnant of a supernova explosion just 6500 light years from Earth in our own galaxy.
2006年Integral做了一次相似的觀測，它觀測了距離我們銀河系6500光年的一次超新星爆炸産物——蟹狀星雲(yún)，測量了其偏振輻射。
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,爆炸後的賸餘物4,下節(jié)課我會,詳細講它,這裡你看到的不是,脈沖星那時,聚集的物質(zhì)。