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Modelling X-ray and Gamma-ray Emission from Pulsars

Published online by Cambridge University Press:  26 May 2016

B. Rudak  and
J. Dyks
B. Rudak
Affiliation:
Nicolaus Copernicus Astronomical Center, Rabiańska 8, 87-100 Toruń, Poland
J. Dyks
Affiliation:
Nicolaus Copernicus Astronomical Center, Rabiańska 8, 87-100 Toruń, Poland

Abstract

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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.

Type
Part 5 Pulsars and Other Neutron Stars
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 177 - 180
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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