一个高度磁化的长周期无线电短变体,表现出不寻常的发射特征
Yunpeng Men1, Sam McSweeney2, Natasha Hurley-Walker2
1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Bonn, D-53121, Germany.
Science advances
|January 17, 2025
概括
长周期无线电瞬态,如GPM J1839-10,显示不寻常的无线电信号. 这些发现支持长周期磁星模型,并将这些物体与快速无线电爆发 (FRB) 联系起来.
科学领域:
- 天体物理学 天体物理学
- 无线电天文学 无线电天文学
- 短暂的现象是短暂的现象
背景情况:
- 长周期无线电瞬态是新发现的一类天体物理物体.
- 它们的发射在几十分钟的时间尺度上是周期性的,但它们的起源是未知的.
- 潜在的候选者包括磁性白矮星,二进制系统或长周期磁星,它们被认为可以产生快速无线电爆发 (FRB).
研究的目的:
- 为了研究长期无线电瞬态GPM J1839-10的性质.
- 用先进的射电望远镜数据分析其不寻常的发射特性.
- 测试长期磁器模型及其与FRBs的连接.
主要方法:
- 使用MeerKAT射电望远镜对GPM J1839-10进行了后续观测.
- 分析了无线电发射的特性,包括极化和基层结构.
- 将观察到的特征与磁星和FRB的理论预测进行了比较.
主要成果:
- GPM J1839-10 呈现出独特的极化特征,表明其起源于磁层.
- 观察到线性到圆性的偏振转换.
- 检测到类似于重复FRB中观察到的漂移子结构.
结论:
- 观察到的无线电特征提供了强有力的证据,支持GPM J1839-10的长期磁星模型.
- 这些发现表明,长周期无线电瞬态,磁星和快速无线电爆发之间存在潜在联系.
- 需要进一步的研究才能充分理解这些神秘的宇宙现象.
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