In this paper, assuming that pulsar magnetic field is rotating vacuum dipole, which is derived from retarded potential, the PA curve is reinvestigated.

 
  • 文章采用从推迟势导出的旋转真空磁偶极场,研究了在脉冲星磁场为旋转磁偶极场位形下的线偏振位置角曲线。
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