射电脉冲星1822—09微脉冲的性质 |
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作者姓名: | 吴鑫基 金声震 |
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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 |
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基金项目: | Supportcd by National Climbing Program,National Science Fundation |
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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).
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关 键 词: | 射电脉冲星 脉冲 性质 |
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