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 L(张力)1,2; Wu, J2; Jiang, ZJ2; Mei, DC2
刊名CHINESE PHYSICS LETTERS
出版日期2003-03
卷号20期号:3页码:433-435
ISSN号0256-307X
产权排序第一完成单位
通讯作者Zhang, L (reprint author), Chinese Acad Sci, Natl Astron Observ, POB 110, Kunming 650010, Peoples R China.
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 End 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.
WOS标题词Science & Technology ; Physical Sciences
学科主题Physics
类目[WOS]Physics, Multidisciplinary
研究领域[WOS]Physics
关键词[WOS]UNIDENTIFIED EGRET SOURCES ; RAPIDLY SPINNING PULSARS ; POWERED PULSARS ; RADIATION
收录类别SCI
原文出处http://iopscience.iop.org/0256-307X/20/3/335/
语种英语
WOS记录号WOS:000181790000035
源URL[http://ir.ynao.ac.cn/handle/114a53/4169]  
专题云南天文台_其他
作者单位1.National Astronomical Observatories and Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650010
2.Department of Physics, Yunnan University, Kunming 650091
推荐引用方式
GB/T 7714
Zhang L,Wu, J,Jiang, ZJ,et al. Gamma-ray pulsars expected in the outer gap model of gamma-ray emission[J]. CHINESE PHYSICS LETTERS,2003,20(3):433-435.
APA Zhang L,Wu, J,Jiang, ZJ,&Mei, DC.(2003).Gamma-ray pulsars expected in the outer gap model of gamma-ray emission.CHINESE PHYSICS LETTERS,20(3),433-435.
MLA Zhang L,et al."Gamma-ray pulsars expected in the outer gap model of gamma-ray emission".CHINESE PHYSICS LETTERS 20.3(2003):433-435.

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来源:云南天文台

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