Title of article
A study on emission geometry and the separation of peaks in the γ-ray pulse profiles of pulsar Original Research Article
Author/Authors
K.J. Lee، نويسنده , , G.J. Qiao، نويسنده , , H.G. Wang، نويسنده , , R.X. Xu، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2006
Pages
4
From page
1988
To page
1991
Abstract
In the inner annular gap (IAG) model the γ-ray radiation sources are suggested to be located close to the null charge surface (NCS). A method to explore two geometric parameters (κ, λ) of the IAG model is given in this paper. Pulsar population statistics are proposed to test the radiation locations of γ-ray pulsars. Within the IAG model, predictions for the GLAST observation of γ-ray pulsars are also made.
Keywords
Pulsars: general , Radiation mechanisms: non-thermal
Journal title
Advances in Space Research
Serial Year
2006
Journal title
Advances in Space Research
Record number
1130905
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