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Synthesis and Characterization of Supramolecular Colloids
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在吸收中检测到的紫外线暗原团群
Andrew B Newman1, Gwen C Rudie2, Guillermo A Blanc2,3
1Observatories of the Carnegie Institution for Science, Pasadena, CA, USA. anewman@carnegiescience.edu.
Nature
|June 15, 2022
概括
研究人员通过观察星系间气体而发现星系原团, 许多候选原星团含有比预期的更少的星系,这表明由于环境影响而变暗的成员.
科学领域:
- 宇宙学
- 银河系的演变
- 天体物理学
背景情况:
- 星系原团是巨大的星系团的先驱.
- 目前追踪原星团的方法依赖于星系的过度密度,而这些过度密度会受到恒星形成和尘埃的影响.
- 对大质量原星团需要新的追踪器, 独立于星系属性.
研究的目的:
- 在红移2.2-2.8时识别和描述大质量星系原团.
- 研究原始星团环境与星系群体之间的关系.
- 开发使用星际气体追踪原星团的新方法.
主要方法:
- 在背景星系的光谱中观察到莱曼α吸收.
- 用一个厚厚的背景星系网来探测星际气体.
- 根据莱曼α吸收信号定位候选原团.
主要成果:
- 在红移2.2至2.8确定了大量的候选原团.
- 发现最能吸收的结构含有比模拟预测的暗物质含量少的星系.
- 推断一半的预期星系成员在休息紫外线波长时是昏暗的.
结论:
- 星系间气体是巨大的原始星团的有效标志物.
- 原星团环境对早期星系进化产生了重大影响,减少了恒星形成和增加了尘埃.
- 早期的环境影响可能会解释大质量原星团中观测到的星系数量较少.
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