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A Further Study of Relative Longitude Shift of Pulsar Beams
Qiao Guojun; Xu Jianwen; Xu Renxin
2001
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume1Issue:2Pages:152
AbstractIt 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51132
Collection中国科学院国家天文台
Affiliation中国科学院-北京大学联合北京天体物理中心
Recommended Citation
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.
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