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在4.69红移的无线电静静类星体周围的分子气体和尘埃
A Omont1, P Petitjean, S Guilloteau
1Institut d'Astrophysique de Paris-CNRS, France.
Nature
|August 1, 1996
概括
早期的星系迅速形成恒星. 研究人员在一个遥远的类星体中检测到分子气体和尘埃,证实了早期宇宙中存在大质量恒星形成的条件.
科学领域:
- 宇宙进化的宇宙进化.
- 银河系的形成和演变.
- 早期宇宙的天体物理学
背景情况:
- 据认为,星系在其历史早期经历了显著的恒星形成.
- 在红移z>4的类星体中,重元素合成的证据表明早期的分子气体存在.
- 分子气体对于恒星形成至关重要,正如在低红移星系中观察到的.
研究的目的:
- 为了调查遥远星系中分子气体的存在.
- 了解宇宙中早期星爆的条件.
- 探测早期类星体的组成.
主要方法:
- 使用射电天文学检测尘埃和一氧化碳排放.
- 将排放映射到空间分辨的组件.
- 红移分析以确定宇宙距离.
主要成果:
- 在无线电静音类星体BR1202-0725中检测到尘埃和一氧化碳排放,红移z=4.69.
- 绘制地图显示了两个不同的物体,表明伴侣星系或引力透镜.
- 在已知最遥远的星系之一中证实了大量的分子气体质量.
结论:
- 早期的宇宙 (z=4.69) 拥有适合大质量恒星形成的条件.
- 分子气体存在于遥远的类星体中,支持早期星系进化理论.
- 这些发现提供了关于第一个星系的形成和生长的见解.
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