马射线爆发:在早期宇宙中的巨大爆炸
G Cusumano1, V Mangano, G Chincarini
1INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, 90146 Palermo, Italy. cusumano@ifc.inaf.it
Nature
|March 10, 2006
概括
观测到的最遥远的长马射线爆发 (GRB) 发生在128亿年前. 这个宇宙爆炸提供了关于早期恒星形成和年轻宇宙中黑洞发展的见解.
科学领域:
- 天文学和天体物理学
- 宇宙学的宇宙学是什么?
- 高能天体物理学 高能天体物理学
背景情况:
- 长马射线爆发 (GRBs) 是与巨大的恒星崩相关的能量现象.
- 早期宇宙 (大爆炸后大约8.9亿年) 是一个重要的恒星形成和进化的时期.
研究的目的:
- 报告和分析有史以来发现的最遥远的长马射线爆发 (GRB 050904) 的观测结果.
- 研究早期宇宙的条件,特别是恒星形成和黑洞起源,接近再电离时代.
主要方法:
- 利用马和X射线观测来检测和分析GRB 050904.4.
- 确定GRB的红移 (z = 6.29),以确定其距离和年龄.
主要成果:
- 检测到GRB 050904的红移值为6.29,将其起源置于128亿年前的过去.
- 这一事件发生在宇宙大约有8.9亿年的时代,接近宇宙再电离时代.
- 证实了早期宇宙中巨大的恒星进化和黑洞形成的存在.
结论:
- 这种遥远的GRB的观测支持了长GRB的崩模型.
- 证明恒星形成和进化,导致黑洞的产生,在早期宇宙中迅速发生.
- 提供了了解星系演变和再电离时代条件的关键数据.
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