早期大质量热光环中的冷流作为星系形成的主要模式
1Racah Institute of Physics, The Hebrew University, Jerusalem 91904, Israel. dekel@phys.huji.ac.il
Nature
|January 23, 2009
概括
早期宇宙中的大质量星系不仅仅是由合并形成的. 新的研究表明,它们从稳定的冷气流中生长,形成延伸的旋转盘,而不是以球形主导的结构.
科学领域:
- 宇宙学的宇宙学是什么?
- 银河系的形成和进化
背景情况:
- 早期宇宙中的巨大星系表现出强烈的恒星形成.
- 合并事件被认为是这种恒星形成的主要驱动因素.
- 观测到的星系属性,如气体丰富,块状,延伸的旋转盘,往往与合并驱动的形成模型相矛盾.
研究的目的:
- 研究年轻宇宙中大质量星系的气体积聚机制.
- 为了使早期大质量星系的观测属性与理论形成途径相协调.
- 探索一种替代星系形成的融合驱动模型.
主要方法:
- 利用宇宙学模拟来建模星系的形成.
- 应用集群理论来理解气体采集.
- 模拟结果与恒星形成星系的观测数据进行了比较.
主要成果:
- 确定了由稳定,冷的气体流穿透暗物质光环而形成的"流养星系".
- 发现大多数积累的气体迅速转化为恒星.
- 确定平滑流为四分之三的星系以给定的速度形成恒星,而罕见的亚毫米星系的强烈星体爆发是由于合并引起的.
结论:
- 冷气流,而不仅仅是合并,是早期宇宙中大规模星系形成的重要驱动因素.
- 流积累保留了旋转的磁盘结构,允许块,的进化成为球体.
- 这种流动驱动的场景为早期星系组装的合并范式提供了一个可行的替代方案.
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