Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-08T01:56:47.609Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Radiation Characteristics of Pulsars and Magnetic Dipole Angle

Published online by Cambridge University Press:  14 August 2015

Wang Zhen-ru  and
Chu Yi
Wang Zhen-ru
Affiliation:
Department of Astronomy, Nanking University, Nanking, China
Chu Yi
Affiliation:
Department of Astronomy, Nanking University, Nanking, China

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The structure of the pulsar magnetosphere, the location of the radio emission region and the radio emission mechanism are important theoretical subjects in the research of pulsars. There may be close relations between these subjects. Nevertheless, it should be possible to set up some empirical relations among them which can be considered as a foundation for studying these important subjects. In this paper some of these relations are studied.

Type
III. Radio Observations of Pulsars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 217 - 218
Copyright
Copyright © Reidel 1981 

References

Backer, D.C.: 1976, Astrophys. J. 209, p. 895.Google Scholar
Ferguson, D.C.: 1977, Astron. Astrophys. 54, p. 355.Google Scholar
Henry, G.R. and Park, H.J.: 1969, Nature 224, p. 1188.Google Scholar
Lyne, A.G. and Smith, F.G.: 1979, Mon. Not. R. Astr. Soc. 188, p. 675.Google Scholar
Qin-yue, Qu, Zhen-ru, Wang, Tan, Lu, and Liao-fu, Luo: 1976, Kexue Tongbao 21, No. 4, p. 176.Google Scholar