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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: [email protected]
Guo Jun Qiao
Affiliation:
School of Physics, Peking University, Beijing 100871, China email: [email protected]
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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

References

Abdo, A. A., Ackermann, M., Ajello, M., et al. 2009, Science, 325, 848Google Scholar
Abdo, A. A., et al. 2010a, ApJs, 187, 460Google Scholar
Cheng, K. S., Ho, C., & Ruderman, M. 1986, ApJ, 300, 500Google Scholar
Daugherty, J. K. & Harding, A. K. 1994, ApJ, 429, 325Google Scholar
Du, Y. J., Qiao, G. J., Han, J. L., Lee, K. J., & Xu, R. X. 2010, MNRAS, 406, 2671CrossRefGoogle Scholar
Du, Y. J., Han, J. L., Qiao, G. J., & Chou, C. K. 2011, ApJ, 731, 2CrossRefGoogle Scholar
Du, Y. J., Qiao, G. J., & Wang, W. 2011, ApJ, 748, 84Google Scholar
Dyks, J. & Rudak, B. 2003, ApJ, 598, 1201Google Scholar
Zhang, J. L. & Cheng, K. S. 1995, Physics Letters A, 208, 47Google Scholar
Pellizzoni, A., et al. 2009, ApJ, 695, L115Google Scholar
Qiao, G. J., Lee, K. J., Wang, H. G., Xu, R. X., & Han, J. L. 2004, ApJ, 606, L49CrossRefGoogle Scholar
Qiao, G. J., Lee, K. J., Zhang, B., Wang, H. G., & Xu, R. X. 2007, Chin. J. Astron. Astrophys., 7, 496Google Scholar