NAOC Open IR
xrayemissionfromrotationpoweredpulsars
Lin Guifang1; Zhang Li2
2005
Source Publicationchinesephysicsletters
ISSN0256-307X
Volume22Issue:4Pages:1022
AbstractWe study the properties of pulsed component of hard (2-10keV) x-ray emission from pulsars based on the new version of outer gap model we proposed previously Astrophys. J. 604 (2004) 317. On the frame of this outer gap model, we derive an expression of non-thermal pulsed x-ray luminosity of rotation-powered pulsars, and then apply it to the pulsars whose pulsed x-rays are detected by ASCA. Using the Kolmogorov-Smirnov test; we determine the model parameter. The present results indicate L-X proportional to L-sd(1.15) for these x-ray pulsars, which is consistent with the observed data.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/40363
Collection中国科学院国家天文台
Affiliation1.云南大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
Lin Guifang,Zhang Li. xrayemissionfromrotationpoweredpulsars[J]. chinesephysicsletters,2005,22(4):1022.
APA Lin Guifang,&Zhang Li.(2005).xrayemissionfromrotationpoweredpulsars.chinesephysicsletters,22(4),1022.
MLA Lin Guifang,et al."xrayemissionfromrotationpoweredpulsars".chinesephysicsletters 22.4(2005):1022.
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