Statistic of Pulsars in Galaxy disks and Globular Clusters

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• 作者：Zhang C.M.Pan Y.Y.Wang N.
• 会议时间：2012-08-13
• 作者单位：Zhang C.M.(National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China)Pan Y.Y.(National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China;Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Xinjiang 830011, China)Wang N.(National Astronomical Observatories, Chinese Academy of Sciences, Beijing100012, China;Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Xinjiang 830011, China)
• 母体文献：2012年快脉冲星研讨会(FAST2012)论文集
• 会议名称：2012年快脉冲星研讨会(FAST2012)
• 会议地点：乌鲁木齐
• 主办单位：中科院新疆天文台
• 语种：chi

摘要

Investigating the distributions of binary pulsars in globular clusters (GCs) and galaxy disks (GDs),we ˉnd that most of them are located in the mil- lisecond range.The statistic of their spin period,magnetic ˉeld,eccentricity and companion mass show their di?erences.It is deduced that the dynamic mechanism is complicated for forming the BPSRs in GC than in GD.