一个非常明亮的磁力驱动的超新星,与超长的γ射线爆发相关
Jochen Greiner1, Paolo A Mazzali2, D Alexander Kann3
11] Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany [2] Excellence Cluster Universe, Technische Universität München, Boltzmannstrasse 2, 85748 Garching, Germany.
Nature
|July 10, 2015
概括
天文学家发现了一颗超亮超新星 (SN 2011kl),与超长马射线爆发 (GRB 111209A) 有关. 这一事件挑战了现有的超新星模型,并暗示了磁星能量注入.
科学领域:
- 天体物理学 天体物理学
- 宇宙爆炸,宇宙爆炸.
- 马射线天文学 马射线天文学
背景情况:
- 超长时间的马射线爆发 (GRBs) 是最近提出的一类事件.
- 以前的超长GRBs缺乏明确的超新星关联.
- 潜在的起源包括非常大的恒星爆炸或恒星潮干扰.
研究的目的:
- 报告与超长GRB相关的第一个确认的超新星.
- 为了描述这个独特的超新星的特性.
- 调查超长GRBs的祖先和能量来源.
主要方法:
- 观测和分析马射线爆发GRB 111209A及其相关的光学瞬态.
- 对超新星SN 2011kl.的光谱和光度分析.
- 与已知的超新星类型和理论模型进行SN 2011kl属性的比较.
主要成果:
- 一个超新星,SN 2011kl,最终与超长GRB 111209A与红移z=0.677.7的红移有关.
- 超新星SN 2011kl的亮度是典型的Ic型超新星的三倍多.
- 它的光谱与超级发光的超新星有相似之处,但具有明显的紫外线特征,暗示金属度低.
结论:
- SN 2011kl的高亮度和低金属线不透明度挑战了传统的Ic型超新星解释.
- 观察到的特性与一个模型相一致,该模型涉及来自磁铁的能量注入.
- 这一发现为超长GRB及其祖先的性质提供了关键的见解.
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