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年轻脉冲星的X-射线非热辐射
引用本文:靳玉芝.年轻脉冲星的X-射线非热辐射[J].安徽大学学报(自然科学版),2010,34(4).
作者姓名:靳玉芝
作者单位:四川理工学院,物理系,四川,自贡,643000
摘    要:年轻的转动驱动脉冲星有较高的自转能损率(Lsd≥1036erg.s-1),而且都有非常高的非热X-射线辐射,利用新的外间隙模型,计算年轻脉冲星的非热X-射线光度,并与观测到的17颗年轻脉冲星的非热X-射线光度能量范围为2~10 keV的观测结果进行比较,模型的计算结果和观测数据吻合较好.

关 键 词:年轻脉冲星  外间隙模型  X-射线

X-ray non-thermal radiation of young Pulsars
JIN Yu-zhi.X-ray non-thermal radiation of young Pulsars[J].Journal of Anhui University(Natural Sciences),2010,34(4).
Authors:JIN Yu-zhi
Institution:JIN Yu-zhi(Department of Physics,Sichuan University of Science and Engineering,Zigong 643000,China)
Abstract:Young rotation-powered pulsars usually possess large values of the rotational-energy loss(Lsd≥1036 erg·s-1),and have very high non-thermal X-ray radiation.In the frame of the revised outer gap model,study the non-thermal X-ray radiation(energy range 2~10 keV) of seventeen young pulsars observed,the predicted values were consistent with the observed date,and calculate the non-thermal X-ray luminosity of young pulsars with outer gaps.
Keywords:young pulsars  outer gap model  X-ray  
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