The relation between emission beam width (ρ) and period (P) of pulsars is studied via the relation of K-P.
从极冠模型出发,利用观测参数K和辐射锥角的关系,通过研究K-P关系导出了对确定辐射区参数有重要意义的辐射束宽和周期的关系。
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