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arXiv · 1210.5801

Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

YuanJie Du·GuoJun Qiao
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Abstract

The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish our single magnetic pole model from two-pole models (e.g. outer gap model and two-pole caustic model), the convincing values of the magnetic inclination angle and the viewing angle will play a key role.

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YuanJie Du, GuoJun Qiao. 2012-10-22. Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars. https://doi.org/10.1017/s1743921312024180

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