一些星团中过多的软X射线组件的可能星团内部起源
1Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK.
概括
星系团的柔软X射线光谱表明,标准模型无法解释过量的辐射. 一个流混合层模型为星系团中这种过量的软辐射提供了潜在的解决方案.
科学领域:
- 天文学和天体物理学
- 等离子体物理学的物理学
背景情况:
- 星系团从热的星系团内部介质发出X射线.
- 观察到的处女座和昏迷星团的软X射线光谱偏离了标准模型.
- 我们银河系的光电吸收不能完全解释观测到的光谱.
研究的目的:
- 调查来自星系团的过度软X射线辐射的来源.
- 解释观察到的光谱与热内部介质模型之间的差异.
- 提出一个新的模型来解释观察到的软X射线过量.
主要方法:
- 来自处女座和昏迷星系团的软X射线光谱的分析.
- 观察到的光谱与热的集群内部介质和光电吸收模型的比较.
- 开发和评估一个流混合层模型.
主要成果:
- 标准模型无法解释星系团的软X射线光谱.
- 过度的软排放表明冷却气体的热排放 (约. 100万韩元) 的资金.
- 这种气体的快速冷却对其起源和命运提出了挑战.
结论:
- 一个乱的混合层模型可以解释过多的软X射线辐射.
- 这个模型建议在冷却后重新加热气体,保持小的总质量.
- 该模型为星系团中的冷却气体问题提供了潜在的解决方案.
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