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
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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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