Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

	Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars
	Yuan Jie Du ; Guo Jun Qiao
	2012
会议日期	2012
关键词	gamma rays: stars pulsars: general radiation mechanisms: non-thermal
页码	378-380
通讯作者	北京8701信箱
中文摘要	The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish our single magnetic pole model from two-pole models (e.g. outer gap model and two-pole caustic model), the convincing values of the magnetic inclination angle and the viewing angle will play a key role.
会议录	Proceedings of the International Astronomical Union
学科主题	空间技术
语种	英语
内容类型	会议论文
源URL	[http://ir.cssar.ac.cn/handle/122/572]
专题	国家空间科学中心_空间技术部
推荐引用方式 GB/T 7714	Yuan Jie Du,Guo Jun Qiao. Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars[C]. 见:. 2012.