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A full polar cap cascade model: pulsar γ-ray and X-ray luminosities
Published online by Cambridge University Press: 12 April 2016
Abstract
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We propose a full polar cap cascade model which includes the curvature and inverse Compton emission of the primary particles, and both synchrotron radiation and inverse Compton of the higher generation pairs. Such a full cascade model can reproduce both the Lγ ∝ (Lsd)1/2 and the Lx ~ 10−3Lsd dependences observed from the known spin-powered pulsars.
- Type
- Part 6. Emission and Plasma Theory
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 481 - 482
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Thompson, D.J., Harding, A.K., Hermsen, W., & Ulmer, M.P.
1997, in Dermer, C.D., Strickman, M.S., & Kurfess, J.D. (eds.), Proc. Fourth Compton Symposium, AIP Conf. Proc.
410, 39
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