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Updated: Jun 25, 2025

11:47
A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
Published on: December 22, 2018
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在X射线爆发之后,一个自由预处理的磁星
Gregory Desvignes1,2, Patrick Weltevrede3, Yong Gao4,5
1Max-Planck-Institut für Radioastronomie, Bonn, Germany.
概括
磁体,高度磁化的中子星,可能不会导致重复的快速无线电爆发 (FRB). 新的观测表明,它们的前行减湿太快,挑战了这种FRB起源理论.
科学领域:
- 天文学和天体物理学
- 高能天体物理学 高能天体物理学
- 中子星物理学 中子星物理学
背景情况:
- 磁星,高度磁化的中子星,是快速无线电爆发 (FRB) 的首要候选人.
- 假设重复的FRB来自自由预处理磁星.
研究的目的:
- 为了调查磁星在X射线爆发后自由前行的潜在作用.
- 测试假设自由预处理磁星是重复FRBs的起源.
主要方法:
- 在X射线爆发后对磁星XTE J1810-197进行了高频率无线电观测.
- 分析了磁星的无线电发射中的极化变化.
- 应用了具有衰减摇摆角度的自由前行模型.
主要成果:
- 观察到的极化变化与磁体自由前行和磁层解相一致.
- 发现观察到的前置在几个月的时间尺度上减弱.
- 磁星圆度的测量与核物理学的理论预测一致.
结论:
- precession 的快速缓解反对自由预处理磁器作为重复FRBs 的来源.
- 该研究提供了磁星几何学的精确测量,有助于X射线光曲线建模和紧性约束.
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