GRB 130427A:一个附近的普通怪物
A Maselli1, A Melandri, L Nava
1Istituto Nazionale di Astrofisica (INAF)-Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF) Palermo, Via Ugo La Malfa 153 I-90146 Palermo, Italy.
概括
长时间的马射线爆发 (GRBs) 是罕见的恒星崩事件. GRB 130427A,一个附近和明亮的例子,提供了关于推动这些宇宙爆炸在整个宇宙中的引擎的见解.
科学领域:
- 天体物理学 天体物理学
- 宇宙爆炸,宇宙爆炸.
- 恒星进化中的恒星演变
背景情况:
- 长时间的马射线爆发 (GRBs) 是来自大质量恒星崩的罕见,强大的爆炸.
- 它们通常是在遥远的宇宙中观察到的,这使得详细的研究具有挑战性.
- GRB 130427A是一个非常明亮和相对接近的事件 (z = 0.34).
研究的目的:
- 为GRB 130427A.提供全面的多波长分析.
- 了解从提示到后照相阶段的排放演变.
- 通过宇宙时间调查负责GRBs的中央引擎.
主要方法:
- 利用了来自Swift天文台的数据.
- 纳入了利物浦和福克斯望远镜的观测结果.
- 来自各种其他地面设施的综合数据.
主要成果:
- GRB 130427A在马射线波段中表现出观察到的最高流动度.
- 详细的多波长观测涵盖了提示和后发光阶段.
- 爆发的属性与高亮度,高红移GRB的属性保持一致.
结论:
- GRB 130427A提供了一个独特的附近实验室来研究GRB物理.
- 一个共同的中央发动机可能为跨越宇宙时代和能量范围的GRB提供动力.
- 这一发现表明了长时间GRBs起源的统一模型.
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