来自活跃银河系核的热气泡作为冷却流集群中的热源
Marcus Brüggen1, Christian R Kaiser
1International University Bremen, Campus Ring 1, 28759 Bremen, Germany. m.brueggen@iu-bremen.de
Nature
|July 19, 2002
概括
星系团中的活跃星系核膨胀浮力气泡. 这些气泡起热气体,增加冷却时间并减少冷气沉积,与以前的冷却流模型相反.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 等离子体物理学的物理学
背景情况:
- 星系团包含热的,发射X射线的等离子体.
- 观察到的中央X射线亮度峰值表明气体冷却流.
- 预测和观察到的冷气之间存在差异,这意味着质量沉积率较低.
研究的目的:
- 研究活跃星系核 (AGN) 对星系团气体冷却的影响.
- 根据AGN活动,重新评估冷却流量模型.
- 量化浮力气泡对气体热力学的影响.
主要方法:
- 高分辨率的水力动力学模拟.
- 模拟AGN膨胀的等离子泡.
- 分析模拟集群核心中的气体和冷却时间.
主要成果:
- 浮力气泡通过集群大气层上升,动气体.
- 模拟显示内部集群区域的冷却时间增加.
- 由于泡活动,冷气沉积的显著减少.
结论:
- 由AGN驱动的浮力气泡在调节星系团中的气体冷却方面发挥着至关重要的作用.
- 如果不考虑AGN反,冷却流量模型可能是不完整的.
- 这些发现协调了观察到的冷气量的差异.
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