X-Ray Polarimetry Workshop SLAC, Stanford, California 9-11 February 2004

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Pulsar polarization from the outer gap

Roger

Romani

Stanford University

rwr@astro.stanford.edu

Roger W. Romani

I present a brief review of the polarization signatures expected for pulsar non-thermal emission from the outer magnetosphere. The potential X-ray polarizations are compared to lower (radio, optical) and higher (Gamma-ray) energies.

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For more information, contact Jennifer Formichelli
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