As these tiny stellar remnants orbit one another, calculations show that they should lose energy and spiral together.
一旦这些微小的恒星遗存互相围绕运行,计算表明它们将失去能量盘旋接近。
Besides supernova remnants, these shock models are important in understanding a wide range of astrophysical phenomena, ranging from winds in newly-formed stars to cataclysmic stellar outbursts.
除了残骸,这些冲击波模型对于了解一系列天体物理学现象,从新恒星上的气体流动到恒星物质的喷发,有很重要的帮助。
Supernova remnants play an important role in stellar evolution by enriching space with heavy elements, and triggering new star formation by compressing interstellar gas.
超新星残骸以重元素填充宇宙空间,压缩星际气体促进新恒星的形成,因而在星体演化过程中扮演重要角色。
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