一个与短时间的gamma射线爆发GRB 130603B相关的"基隆新星"
N R Tanvir1, A J Levan, A S Fruchter
1Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK. nrt3@le.ac.uk
Nature
|August 6, 2013
概括
短时间的马射线爆发 (GRBs) 与紧物体的合并有关. 对GRB 130603B的观测显示了一个千新星,证实了合并作为GRB起源和r-process元素地点.
科学领域:
- 天体物理学 天体物理学
- 核天体物理学 核天体物理学
- 宇宙马射线爆炸
背景情况:
- 短时间的马射线爆发 (GRBs) 是短暂的,强烈的宇宙射线闪光.
- 它们的起源是有争议的,紧物体的合并是主要假设.
- 预计合并会产生富含中子元素和千新星.
研究的目的:
- 为了确认短时间GRBs的原始模型.
- 为了调查r-process元素的起源.
- 为了识别千新星作为合并的电磁对应物.
主要方法:
- 对GRB 130603B的光学和近红外观测.
- 在GRB之后的短暂发射的分析.
- 观察结果与千新星理论模型的比较.
主要成果:
- 强有力的证据表明,一颗伴随GRB 130603B的千新星.
- 观测到的排放与由放射性衰变驱动的千新星的预测相匹配.
- 事件的能量分布与近红外辐射相一致.
结论:
- 紧物体的合并被证实是短时间GRBs的祖先.
- 这些合并是生产r工艺元件的重要地点.
- 千诺瓦为引力波源提供了替代的电磁特征.
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