A Further Study of Relative Longitude Shift of Pulsar Beams
文献类型：期刊论文
| 作者 | Qiao Guojun; Xu Jianwen; Xu Renxin |
| 刊名 | Chinese Journal of Astronomy and Astrophysics
 |
| 出版日期 | 2001 |
| 卷号 | 1期号:2页码:152 |
| ISSN号 | 1009-9271 |
| 英文摘要 | It is of great importance to study pulsar beam shape if we are concerned with emission theories and pulsar birth rate. Both observations and the ICS model show that different emission components are emitted from different heights. The relative longitude phase shifts due to different heights of the emission components and the toroidal velocity of the electrons are considered in this paper. Several possible observational effects arising from the phase shift are presented. The emission beams may not have circular cross section although the emission region may be symmetric with respect to the magnetic axis. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/51131]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 中国科学院-北京大学联合北京天体物理中心 |
| 推荐引用方式 GB/T 7714 | Qiao Guojun,Xu Jianwen,Xu Renxin. A Further Study of Relative Longitude Shift of Pulsar Beams[J]. Chinese Journal of Astronomy and Astrophysics,2001,1(2):152. |
| APA | Qiao Guojun,Xu Jianwen,&Xu Renxin.(2001).A Further Study of Relative Longitude Shift of Pulsar Beams.Chinese Journal of Astronomy and Astrophysics,1(2),152. |
| MLA | Qiao Guojun,et al."A Further Study of Relative Longitude Shift of Pulsar Beams".Chinese Journal of Astronomy and Astrophysics 1.2(2001):152. |
入库方式： OAI收割
来源：国家天文台
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