银河系的演化. 银河系的演化. 嵌入巨星星云中的四星四重奏揭示了遥远宇宙中罕见的大质量结构
Joseph F Hennawi1, J Xavier Prochaska2, Sebastiano Cantalupo3
1Max-Planck-Institut für Astronomie, Heidelberg, Germany. joe@mpia.de.
概括
天文学家发现了一种罕见的四重类星体系统,这表明巨星云和原星团之间存在联系. 这一发现挑战了当前关于早期宇宙气体供应的宇宙学模拟.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 银河系的形成和进化
背景情况:
- 星系通过由超大质量黑洞积聚驱动的超发光类星体相进化.
- 类星体相很短,使得类星体很少见,并且通常在宇宙中被广泛分离.
研究的目的:
- 为了研究类星体在大型结构中的关联.
- 探索莱曼-α星云在巨型星系团形成中的作用.
主要方法:
- 在红移 z ≈ 2 时对莱曼-α 辐射进行了调查.
- 在一个巨大的星云中确定了四个类星体的物理联系.
- 分析了周围银河系的过度密度,以评估系统的性质.
主要成果:
- 在一个巨大的星云中发现了一个独特的四重类星系统.
- 该系统位于一个显著的星系过度密度,可能是原始星团的祖先.
- 这种四重类星体偶然出现的概率非常低 (∼10(-7)).
结论:
- 莱曼-阿尔法星云与罕见原始星团的地点有物理联系.
- 早期宇宙中的巨大结构拥有大量的冷,密集的气体储备 (∼10~11太阳质量).
- 这种气体供应与当前宇宙学模拟的预测相矛盾.
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