Polarization of pulsar radiation in the two-pole caustic model and in the outer gap model

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dc.creatorDyks, J.
dc.creatorHarding, A. K.
dc.creatorRudak, B.
dc.date2004-03-17
dc.date.accessioned2026-07-07T02:12:39Z
dc.date.available2026-07-07T02:12:39Z
dc.descriptionWe present linear polarization characteristics of pulsar radiation as predicted by two models of high-energy radiation from extended regions in the outer magnetosphere: the recently proposed two-pole caustic model, and the outer gap model.
dc.description11 pages, 7 figures, poster presented at the X-ray Polarimetry Workshop, SLAC, Stanford, California, 9 - 11 February 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0403428
dc.identifierhttp://arxiv.org/abs/astro-ph/0403428
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7528
dc.subjectAstrophysics
dc.titlePolarization of pulsar radiation in the two-pole caustic model and in the outer gap model
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