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脱落的超新星光线曲线为中心发动机活动辩护
Ósmar Rodríguez1, Ehud Nakar2, Dan Maoz1
1School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv, Israel.
Nature
|April 17, 2024
概括
剥离外超新星可能具有非放射性电源. 分析了54个超新星, 表明一个中央引擎, 可能形成磁星,
科学领域:
- 天文学与天体物理学
- 恒星进化
- 超新星物理学
背景情况:
- 剥离外超新星 (SESNe) 是一个常见的恒星爆炸.
- 它们的亮度主要归因于放射性衰变.
- 之前的研究提出了额外的能源,但缺乏统计意义或依赖于模型.
研究的目的:
- 调查SESNe的能源预算.
- 在SESNe中找到非放射性电源的观测证据.
- 限制潜在的中央发动机的性能.
主要方法:
- 分析了54个经过充分观察的能源预算.
- 独立于模型的观测比较.
- 评估可能的能源和系统错误.
主要成果:
- 在大多数SESNe中存在非放射性电源的统计学显著证据.
- 这种动力源很可能源于长寿命的中央发动机 (爆炸后10^3-10^6秒).
- 如果发动机是磁器,则初始磁场为1015G,旋转周期为1-100毫秒.
结论:
- 它们很可能拥有超越放射性衰变的核心引擎.
- 这种引擎可能是形成磁星的原因.
- 进一步的研究可以完善这些发动机的性能.
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