在星系间介质的低密度区域中进行重元素丰富
1Institute for Astronomy, University of Hawaii, Honolulu 96822, USA. cowie@uhifa.ifa.hawaii.edu
Nature
|July 17, 1998
概括
早期的星系意外地以重元素丰富了低密度的星系间气体. 这一发现挑战了宇宙化学进化的模型,并表明小星系有效地将元素射出到星系间介质中.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 星系间介质 星系间介质
背景情况:
- 宇宙学模型预测,在高红移时,低密度的星系间气体是元素贫乏的.
- 据认为,重元素的合成和分布主要发生在密集的区域.
研究的目的:
- 在红移三的低密度星际气体中探测重元素的丰度.
- 分析类星光谱中的碳和氧吸收线.
主要方法:
- 开发了一种新的方法来分析类星体光谱中的吸收线.
- 专注于碳和氧吸收线来确定重元素的丰度.
- 检查了各种密度的气体,包括接近零密度的区域.
主要成果:
- 三倍电离碳与中性的比率在各种密度上保持相对不变.
- 即使在接近零密度的地区,重元素的丰度也出乎意料地高.
- 这表明,低密度的星系间气体得到了显著的丰富.
结论:
- 早期的小星系可能非常有效地将重元素喷射到星系间介质中.
- 目前的星系间介质组成模型可能需要修订.
- 建议对早期宇宙化学丰富过程进行修订的理解.
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