解决银河系外的硬X射线背景
Nature
|April 13, 2000
概括
研究人员已经确定了硬X射线背景的来源,几十年来一直是宇宙神秘. 深度卫星的观测显示,这些来源与背景相匹配.
科学领域:
- 宇宙X射线天文学宇宙X射线天文学
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
背景情况:
- 35多年来,硬X射线背景 (2-10 keV) 的起源仍然无法解释.
- 虽然已经确定了软X射线背景源 (主要是类星体),但它们的光谱能量分布与整个背景光谱不匹配.
研究的目的:
- 为了调查和解决硬X射线背景起源的奥秘.
- 识别导致硬X射线背景的来源并分析它们的属性.
主要方法:
- 利用Chandra卫星进行深度X射线调查.
- 分析了检测到的硬X射线源的光谱能量分布.
主要成果:
- 检测到的硬X射线源至少占硬X射线背景的75%.
- 这些源的平均光谱能量分布与背景光谱非常接近.
- 已识别的源与明亮星系的核或光学微弱的物体,潜在的活跃星系核或高红移类星相有关.
结论:
- 这项研究显著解决了长期以来关于硬X射线背景的.
- 确定的来源为观察到的硬X射线背景光谱提供了强有力的解释.
- 这些发现表明,活跃的银河系核,可能是隐藏的或遥远的类星体的显著贡献.
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