The Annular Gap: Gamma-Ray & Radio Emission of Pulsars
文献类型:会议论文
作者 | Qiao G.J.Du Y.J. ; Han J.L. ; Xu R.X. |
出版日期 | 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. |
学科主题 | 空间技术 |
会议录出版地 | Singapore |
语种 | 英语 |
ISSN号 | 2010-1945 |
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. |
入库方式: OAI收割
来源:国家空间科学中心
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。