气体流 gas stream
- 最终的结果是一股持续的气体流,开始是星系间的热气体,结束时是一股被称为“冷却流”的少量冷气体,落入星系中央。
The net result is a continuous flow of gas, starting as hot gases in intergalactic space and ending as a drizzle of cool gas called a "cooling flow," falling into the central galaxy. - 在这些之外还有太阳风——由日冕而来的气体流。
Beyond that is the solar wind, an outflow of gas from the corona. - 最顶层的是超热日冕,由日冕环和电离气体流组成。
At the top is the super-hot corona, which is made of structures such as loops and streams of ionized gas.
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