Variability analysis of EGRET gamma-ray sources

doi:10.1088/1009-9271/5/3/005

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	Variability analysis of EGRET gamma-ray sources
	Han, ZX 1; Zhang L(张力)1,2 ; Han, ZX (reprint author), Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China.
发表期刊	CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
	2005
卷号	5 期号:3 页码:256-264
DOI	10.1088/1009-9271/5/3/005
产权排序	第2完成单位
收录类别	SCI
关键词	Gamma-rays : Observations Galaxies : Statistics Stars : Variables
摘要	The variability of gamma-ray sources listed in the third EGRET catalog is studied using three variability indices. These indices are found to be statistically equivalent if the observed data are sufficiently accurate. Using the three indices, 30 EGRET point sources which are positionally coincident with pulsars and 40 persistent unidentified sources at low latitudes are analyzed for their variability status. It is found that 14 of the 30 point sources may have genuine or plausible associations with pulsars, and 16 of the 40 persistent unidentified sources are possible pulsar candidates.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	1009-9271
URL	查看原文
WOS记录号	WOS:000230099500005
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	GALACTIC PLANE ; PULSARS ; DISCOVERY ; EMISSION ; CATALOG
引用统计	被引频次：2[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/4192
专题	其他
通讯作者	Han, ZX (reprint author), Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China.
作者单位	1.Department of Physics, Yunnan University, Kunming 650091 2.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011
推荐引用方式 GB/T 7714	Han, ZX,Zhang L,Han, ZX . Variability analysis of EGRET gamma-ray sources[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2005,5(3):256-264.
APA	Han, ZX,Zhang L,&Han, ZX .(2005).Variability analysis of EGRET gamma-ray sources.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,5(3),256-264.
MLA	Han, ZX,et al."Variability analysis of EGRET gamma-ray sources".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 5.3(2005):256-264.

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