| Автор | Xu, Ren-Xin |
| Автор | Xu, Jian-Wen |
| Автор | Qiao, Guo-Jun |
| Дата выпуска | 2001-04-01 |
| dc.description | 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. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Копирайт | © 2001 IOP Publishing Ltd |
| Название | A Further Study of Relative Longitude Shift of Pulsar Beams |
| Тип | paper |
| DOI | 10.1088/1009-9271/1/2/152 |
| Print ISSN | 1009-9271 |
| Журнал | Chinese Journal of Astronomy and Astrophysics |
| Том | 1 |
| Первая страница | 152 |
| Последняя страница | 160 |
| Аффилиация | Xu, Ren-Xin; CAS-PKU Joint Beijing Astrophysical Center and Department of Astronomy, Peking University, Beijing 100871 |
| Аффилиация | Xu, Jian-Wen; CAS-PKU Joint Beijing Astrophysical Center and Department of Astronomy, Peking University, Beijing 100871 |
| Аффилиация | Qiao, Guo-Jun; CAS-PKU Joint Beijing Astrophysical Center and Department of Astronomy, Peking University, Beijing 100871 |
| Выпуск | 2 |
