Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars
Proceedings of the International Astronomical Union(2012)
摘要
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. © 2013 International Astronomical Union.
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关键词
gamma rays: stars,pulsars: general,radiation mechanisms: non-thermal
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