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在脉冲星中产生无线电波
1University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank.
Nature
|December 5, 1970
概括
脉冲星通过未知的机制发射强大的无线电波,产生宇宙中最明亮的辐射. 本文详细介绍了脉冲星发射的可观测特征,任何科学理论都必须考虑这些特征.
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
背景情况:
- 脉冲星是高度磁化的旋转中子星,它们发出电磁辐射束.
- 脉冲星中的无线电发射机制仍然是天体物理学中最重要的未解决的问题之一.
- 脉冲星的发射具有极高的体积发射率,超过所有已知的天体物理来源.
研究的目的:
- 编制和呈现有关脉冲星无线电辐射的关键观测事实.
- 为成功的排放理论必须解释的特征提供全面的概述.
主要方法:
- 关于脉冲星无线电辐射的已确定的观测数据的汇编.
- 分析辐射束的特性,包括宽度和极化.
- 对脉冲星光束的频率独立特征的审查.
主要成果:
- 脉冲星无线电发射束的宽度和极化与频率不变.
- 脉冲星所观察到的发射率是已知的天体物理现象中最高的.
- 为脉冲星发射理论组建了一套一致的观测约束.
结论:
- 了解脉冲星无线电发射的基本过程对于天体物理学至关重要.
- 编制的观测事实是验证脉冲星发射理论模型的基本标准.
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