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Spatial Separation of Molecular Conformers and Clusters
Published on: January 9, 2014
星团圆星系的形成是由广泛的恒星形成所揭示的
J A Stevens1, R J Ivison, J S Dunlop
1Astronomy Technology Centre, Royal Observatory, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK. as@roe.ac.uk
Nature
|September 19, 2003
概括
星系团中的巨大星系在早期的宇宙时代迅速形成恒星. 深度亚毫米测绘揭示了以前未被发现的伴星系,支持原星团中同步星系形成的模型.
科学领域:
- 宇宙进化的宇宙进化.
- 银河系的形成和演变.
- 观测天体物理学是一种观测天体物理学.
背景情况:
- 当今宇宙中的巨大星系居住在丰富的星系团中心.
- 这些星系表现出古老的恒星群体,表明早期宇宙时代的恒星形成是显著的.
- 星系形成模型预测大质量星系起源于早期宇宙中的高密度峰值,通常与原始星团相关联.
研究的目的:
- 研究高红移射射电星系及其环境中的恒星形成活动.
- 测试银河系形成模型关于大质量圆星系起源的预测.
- 为了识别和描述当今大质量星系团星系的潜在祖先星系.
主要方法:
- 七个高红移无线电星系及其周围环境的深度亚毫米测绘.
- 检测和分析亚毫米辐射以确定恒星形成活动.
- 观测数据与星系形成模型的比较.
主要成果:
- 在目标高红移射射电星系内确认了大规模恒星形成的空间延伸区域.
- 发现了以前未被发现的伴星系,表现出显著的恒星形成活动.
- 观测到这些伴星系的分布,方向,以及推断到这些伴星系的质量.
结论:
- 这些发现支持原始星团中同步星系形成的模型.
- 这项研究提供了观察证据,证明了星系群体的早期聚集,进化为当今的大型圆星系.
- 亚毫米观测对于揭示早期宇宙中隐藏的恒星形成至关重要.
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