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射电脉冲星1822—09微脉冲的性质
作者姓名:吴鑫基 金声震
作者单位:Department of Geophysics,University of Peking,Beijing,China United Laboratory for Radio Astronomy,Chinese Academy of Sciences,Beijing Astronomical Observatory,Beijing,China,Department of Applied Mathematics Theoretical Physics,University of Cambridge,U.K. National Institute for Space Research-INPE,Brazil,Beijing Astronomical Observatory,Beijing,China
基金项目:Supportcd by National Climbing Program,National Science Fundation
摘    要:The relation between intensity and duration time of micropulses for PSR 1822-09 is studied for comparison with the nonlinear temporal model. The product of intensity and duration lime of micropulses is roughly constant (SpT= 1035 0.2 ). Such relation is consistent with theoretical predictions of the nonlinear temporal model proposed by Chian and Kennel (1983).

关 键 词:射电脉冲星 脉冲 性质
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