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
天体物理喷流,来自恒星和星系的巨大宇宙外流,表现出巨大的尺寸变化. 研究它们的属性为银河系和类星体强大的中央引擎提供了关键的见解.
科学领域:
- 天体物理学 天体物理学
- 太空喷气式飞机 宇宙喷气式飞机
- 银河系的进化 银河系的进化
背景情况:
- 天体物理喷流是巨大的线性结构,起源于恒星和星系.
- 星系喷流是宇宙中最大的结构之一,超过银河系大小100倍.
- 恒星喷射由离子化气体组成,以每秒数百公里的速度移动.
研究的目的:
- 为了定义银河系外喷气的特性.
- 了解银河系外喷气的组成和速度.
- 为了限制星系和类星体中中央动力源的模型.
主要方法:
- 通过与环境介质的相互作用来分析喷气的特性.
- 超银河系喷气组成的特征 (相对论粒子,磁场,等离子体).
- 估计初始外流速度和能量流量.
主要成果:
- 银河系外喷流包含相对论粒子,磁场和等离子体.
- 流出速度可以是相对论的,平均每秒几千公里.
- 能量流可以超过每秒10~46 ergs.
结论:
- 源自环境介质相互作用的喷气特性是关键.
- 这些属性为银河系和类星体电源模型提供了必要的约束.
- 了解天体物理喷射对于理解极端宇宙现象至关重要.
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