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磁器中的一个防故障装置
R F Archibald1, V M Kaspi, C-Y Ng
1Department of Physics, McGill University, Montreal, Quebec H3A 2T8, Canada.
Nature
|May 31, 2013
概括
磁体,高度磁化的中子星,通常在故障时旋转起来. 研究人员观察到一种罕见的磁星倒转"反故障",挑战了当前关于中子星行为的理论.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 恒星物理 恒星物理
背景情况:
- 磁星是具有强大的磁场的中子星,呈现X射线和马射线爆发.
- 中子星,包括磁星和射电脉冲星,经历"故障"突然的旋转事件,归因于地和超流体内部之间的角运动量转移.
研究的目的:
- 为了调查磁星故障的现象,特别关注一个不寻常的倒转事件.
- 分析伴随的X射线变化和与观察到的反故障相关的自转速率变化.
主要方法:
- 对磁星1E 2259+586.6进行了X射线计时观测.
- 分析了时间数据,以检测和描述回转事件和相关的辐射变化.
主要成果:
- 在磁星1E 2259+586中观察到一个明显的"反故障"事件,其特点是突然旋转.
- 反故障事件伴随着多个X射线辐射变化和磁星倒转速率的显著变化.
结论:
- 观察到的回转向下的行为挑战了现有的中子星回转向下的模型.
- 这一事件表明磁星内部的微分旋转,需要对所有中子星的故障理论进行重新评估.
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