Pulsar Observations at Nanshan

来源 :2015 Pulsar and Gravitational- Wave School (脉冲星和引力波学派研讨会) | 被引量 : 0次 | 上传用户：ayun33

【摘要】

：

脉冲星中等质量恒星演化到晚期,超新星爆发产物.已知2524颗脉冲星(还包括磁星、旋转射电暂现源RRAT),绝大多数在银河系.非吸积,自转供能,磁星磁场供能.超高密度、超强磁场引

【作者】

：

袁建平

【机构】

：

中国科学院新疆天文台

【出处】

：

2015 Pulsar and Gravitational- Wave School (脉冲星和引力波学派研讨会)

【发表日期】

：

2015年10期

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脉冲星中等质量恒星演化到晚期,超新星爆发产物.已知2524颗脉冲星(还包括磁星、旋转射电暂现源RRAT),绝大多数在银河系.非吸积,自转供能,磁星磁场供能.超高密度、超强磁场引力场.周期～1s(1.396 ms-11.79 s) 自转减慢 10-15 s/s(1.17x10-21 4.49×10-10 s/s 非热辐射,辐射束

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Pulsar Observations at Nanshan

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