相关实验视频
Updated: Jul 12, 2026

08:34
Cryogenic Liquid Jets for High Repetition Rate Discovery Science
Published on: May 9, 2020
概括
巨大的银河系外无线电源需要持续的能量. 观测表明缓慢移动的冷气流,而不是相对论速度,解释了它们的特性.
科学领域:
- 天体物理学 天体物理学
- 银河系外天文学 银河系外天文学
- 宇宙喷气式飞机 太空喷气式飞机
背景情况:
- 巨大的银河系外无线电源需要不断的能量供应.
- 理论上,能量输入来自银河系和准恒星物体中心,通过气体流或喷气流.
研究的目的:
- 为了研究从银河系外的无线电源发出的喷射的速度和组成.
- 为了使观察到的喷气特性与理论模型相协调.
主要方法:
- 对光学和无线电波长的观测数据的分析.
- 观察到的喷气特征与缓慢移动,流喷气的模型进行比较.
主要成果:
- 发现大型喷气结构以非相对论速度移动.
- 缓慢移动的喷气式飞机具有乱的内部和冷气组成,可以准确地预测观察到的喷气式飞机特性.
- 在能源源附近极小规模喷气的运动仍然不确定.
结论:
- 银河系外无线电源喷流的特性最好用缓慢移动的,动荡的气体流来解释.
- 挑战了以前对大规模喷气式飞机相对论速度的假设.
- 需要对靠近中央能源的小规模喷气进行进一步的研究.
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