Statistical analysis of the radio luminosity of pulsars

Wang Zhen-ru, Qu Qin-yue, Lu Tan, Luo Liao-fu
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引用次数: 4

Abstract

The results of statistical analyses of the radio luminsotiy of 81 pulsars obtained in this paper appear to be in favour of the view that the radio emission originates in regions close to the light cylinder. The various statistical relations given in TABLES 1 and 2 may provide some clues on the radio emission.

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脉冲星射电光度的统计分析
本文对81颗脉冲星的射电光度进行了统计分析,结果似乎支持这样的观点,即射电辐射起源于靠近光柱的区域。表1和表2中给出的各种统计关系可以提供有关无线电发射的一些线索。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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