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Modelling X-ray and Gamma-ray Emission from Pulsars
Published online by Cambridge University Press: 26 May 2016
Abstract
Lightcurves and broadband energy spectra of the brightest X/γ-ray sources among the rotation powered pulsars exhibit unexpected richness of features, making each object almost a unique case. This contribution presents how our models of high-energy radiation within the framework of SCLF (space charge limited flow) polar-cap scenarios tackle with some of these challenges.
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- Part 5 Pulsars and Other Neutron Stars
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- Copyright © Astronomical Society of the Pacific 2003