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Updated: Jul 28, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
一个不对称的能量型Ic超新星被视为离轴,以及与玛射线爆发的联系
Paolo A Mazzali1, Koji S Kawabata, Keiichi Maeda
1Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan. mazzali@ts.astro.it
概括
类型Ic超新星爆炸与马射线爆发有关. 对超新星SN 2003jd的新观测显示,其爆炸是非球形的,为不对称超新星提供了直接证据.
科学领域:
- 天文学和天体物理学
- 超新星和马射线爆炸
背景情况:
- 类型Ic超新星是由缺乏和外的大质量恒星的核心崩造成的.
- 这些超新星特别有趣,因为它们与长时间的马射线爆发 (GRB) 有关.
- 以前的迹象表明存在无球体爆炸,但缺乏直接证据.
研究的目的:
- 为Ic型超新星爆炸的无球性提供直接证据.
- 分析超新星SN 2003jd的晚期观测,以了解其爆炸几何.
- 为了调查SN 2003jd与马射线爆发的潜在关联.
主要方法:
- 使用苏巴鲁和凯克望远镜利用超新星SN 2003jd的晚期光谱观测.
- 对中性氧和的星云线进行分析,以确定其特征.
- 模拟了观察到的光谱形状,以推断爆炸的几何形状.
主要成果:
- 在SN 2003jd.中观测到中性氧和的星云线上的双峰形状.
- 这些形状与其他已知的Type Ic超新星的形状有很大不同,有或没有GRBs.
- 从赤道平面附近观察到的无球,轴对称的爆炸,观察到的配置是一致的.
结论:
- 超新星SN 2003jd提供了Ic型超新星中无球体爆炸的直接证据.
- 观察到的不对称性支持核心崩超新星模型.
- 如果与GRB相关,那么爆发可能是远离地球的.
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