一个无线电短暂的异常缓慢的周期性发射
N Hurley-Walker1, X Zhang2,3, A Bahramian4
1International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, Western Australia, Australia. nhw@icrar.org.
天文学家发现了来自银河系的罕见无线电信号. 这种不寻常的极化瞬态每18分钟就会重复,
科学领域:
- 无线电天文学
- 天体物理学
- 短暂的天文事件
背景情况:
- 低频无线电天空在很大程度上是未经探索的,
- 低频率对来自天体的奇特无线电发射过程敏感.
研究的目的:
- 分析以前未被发现的短暂源的低频无线电数据.
- 描述新发现的周期性无线电瞬态的性质和来源.
主要方法:
- 对档案低频无线电数据的分析.
- 测量脉冲分散以确定源位置.
- 脉冲特性 (周期性,极化,持续时间,形状演变) 的表征.
主要成果:
- 发现一个周期性的低频无线电瞬态.
- 这个源具有18.18分钟的独特周期性.
- 辐射具有高度线性极化,明亮,并且在广泛的频率范围内观察到.
- 源头位于银河系内.
结论:
- 观察到的属性表明,这可能是一个超长周期磁星.
- 这一发现为探测低频无线电频谱中的奇异现象开辟了新的途径.
- 需要进一步的观察来证实磁星假设.
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