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Published on: July 12, 2017
在巨型的无线电脉冲期间增强光学发射
A Shearer1, B Stappers, P O'Connor
1National University of Ireland, Galway, Newcastle Road, Galway, Ireland. andy.shearer@nuigalway.ie
概括
来自脉冲星的巨大无线电脉冲与更明亮的光学脉冲相关,这表明增加的电子-正电子等离子体密度导致了这两种现象.
科学领域:
- 脉冲星天体物理学
- 高能天体物理学 高能天体物理学
- 血物理学的等离子体物理学
背景情况:
- 脉冲星是一个经过充分研究的中子星,以发射无线电和光学脉冲而闻名.
- 巨型无线电脉冲 (GRPs) 是一种罕见的,强烈的无线电辐射爆发.
- 没有完全理解GRP与其他排放波长之间的关系.
研究的目的:
- 为了研究来自脉冲星的光学和巨型无线电脉冲发射之间的相关性.
- 为了确定光学发射特性在GRP事件期间是否发生变化.
主要方法:
- 在正常无线电发射和GRP事件期间对光脉冲配置的比较分析.
- 光学脉冲亮度的光度测量. 光学脉冲亮度的光度测量.
主要成果:
- 在光学和巨型无线电脉冲发射之间发现了统计学上显著的相关性.
- 与GRP相吻合的光脉冲平均比正常无线电发射时的光脉冲亮度高3%.
- 在GRPs期间没有观察到光脉冲形状的其他显著变化.
结论:
- 在GRPs期间增加的光学辐射与电子-正子子等离子体密度的增加有关.
- 无论是GRP还是增强光学辐射,都可能源自一个涉及更高等离子体密度的共同机制.
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