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Two-pole Caustic Model for High-energy Radiation from Pulsars — Polarization

Published online by Cambridge University Press:  19 July 2016

Jarosław Dyks ,
Alice K. Harding  and
Bronisław Rudak
Jarosław Dyks
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD 20771, USA
Alice K. Harding
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD 20771, USA
Bronisław Rudak
Affiliation:
Nicolaus Copernicus Astronomical Center, 87-100 Toruń, Poland

Abstract

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We present high-energy light curves and polarization properties of pulsars calculated within the recently proposed two-pole caustic model. The results are compared with the optical data for the Crab pulsar and with predictions of other high-energy pulsar models: the polar cap model, and the outer gap model.

Type
Part 8: Pulsar Electrodynamics and Emission Theory
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 373 - 374
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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