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

Published online by Cambridge University Press:  20 March 2013

Yuan Jie Du  and
Guo Jun Qiao
Yuan Jie Du
Affiliation:
National Space Science Center, Chinese Academy of Sciences, NO.1 Nanertiao, Zhongguancun, Haidian district, Beijing 100190, China email: duyj@nssc.ac.cn
Guo Jun Qiao
Affiliation:
School of Physics, Peking University, Beijing 100871, China email: gjn@pku.edu.cn
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Abstract

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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.

Keywords

gamma rays: starspulsars: generalradiation mechanisms: non-thermal
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 378 - 380
Copyright
Copyright © International Astronomical Union 2013

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