模拟结果再现了环状日冕物质抛射的主要观测特征。
The results demonstrated the main observed characteristics of the loop-like coronal mass ejection.
被抛射的巨大的恒星的数量正好符合真是观测到的O B速逃星数量。
And the number of massive stars ejected this way matches up well with actual observations of ob runaways.
本文讨论以相对论速度抛射的相对论膨胀等离子团的一些几何学和运动学性质。
In this paper some geometric and kinematic features of a plasmon which is expanding and ejected both relativistically are discussed.
Then in your mind, without realizing it, you found the trajectory at all future times.
在你脑海里,你会下意识地,想像出它之后的抛射轨迹
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