中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray Emission

文献类型:期刊论文

作者Zhang Li1; Wu Jie2; Jiang ZeJun2; Mei DongCheng2
刊名Chinese Physics Letters
出版日期2003
卷号20期号:3页码:433
ISSN号0256-307X
英文摘要We study the possibility of high-energy gamma-ray emission from the known 1130 radio pulsars based on the outer gap model of high-energy emission from pulsars. We estimate the fractional size of outer gap, the integrated flux, the gamma-ray luminosity for each known radio pulsar, and find that only 14% of the known radio pulsars are gamma-ray emitters according to the outer gap model. In the sample of possible 156 gamma-ray pulsars, our statistical analysis indicates that the distributions of the spin-down powers and the ages of these pulsars concentrate mainly on 10~(33.5)-10~(39) erg/s and 10~3-10~7 y, respectively. The predictions of gamma-ray pulsars detected by the AGILE and GLAST missions are given.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/39579]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.云南大学
推荐引用方式
GB/T 7714
Zhang Li,Wu Jie,Jiang ZeJun,et al. Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray Emission[J]. Chinese Physics Letters,2003,20(3):433.
APA Zhang Li,Wu Jie,Jiang ZeJun,&Mei DongCheng.(2003).Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray Emission.Chinese Physics Letters,20(3),433.
MLA Zhang Li,et al."Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray Emission".Chinese Physics Letters 20.3(2003):433.

入库方式: OAI收割

来源:国家天文台

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