The Annular Gap: Gamma-Ray & Radio Emission of Pulsars

	The Annular Gap: Gamma-Ray & Radio Emission of Pulsars
	Qiao G.J.Du Y.J. ; Han J.L. ; Xu R.X.
	2013
会议名称	3rd Galileo - Xu Guangqi Meeting
会议日期	2013
会议地点	Beijing, China
关键词	Neutron star quark star magnetosphere non-thermal radiation mechanisms.
页码	21-26
通讯作者	北京8701信箱
中文摘要	Pulsars have been found more than 40 years. Observations from radio to gamma-rays present abundant information. However, the radiation mechanism is still an open question. It is found that the annular gap could be formed in the magnetosphere of pulsars (neutron stars or quark stars), which combines the advantages of the polar cap, slot gap and outer gap models. It is emphasized that observations of some radio pulsars, normal and millisecond gamma-ray pulsars (MSGPs) show that the annular gap would play a very important role. Here we show some observational and theoretical evidences about the annular gap. For example, bi-drifting sub-pulses; radio and gamma-ray millisecond pulsars and so on.
收录类别	SCI
会议录	International Journal of Modern Physics: Conference Series
会议录出版者	World Scientific Publishing Co. Pte. Ltd.
会议录出版地	Singapore
学科主题	空间技术
语种	英语
ISSN号	2010-1945
内容类型	会议论文
源URL	[http://ir.cssar.ac.cn/handle/122/573]
专题	国家空间科学中心_空间技术部
推荐引用方式 GB/T 7714	Qiao G.J.Du Y.J.,Han J.L.,Xu R.X.. The Annular Gap: Gamma-Ray & Radio Emission of Pulsars[C]. 见:3rd Galileo - Xu Guangqi Meeting. Beijing, China. 2013.