The Effect of aberration on polarization position angle of pulsars

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dc.creatorMitra, D.
dc.creatorSeiradakis, J. H.
dc.date2004-01-16
dc.date.accessioned2026-07-07T02:11:53Z
dc.date.available2026-07-07T02:11:53Z
dc.descriptionThe linear polarization position angle (PPA) of pulsar emission shows a wide variety of structures, which deviates from the classical rotating vector model. In this study we investigate the effect on the PPA due to emission arising from a range of heights. We demonstrate that by appropriately choosing the emission height we can reconstruct the PPA sweep across the integrated pulse profiles.
dc.description4 pages, 2 Figures, Proceedings of 6th Hellenic Astronomical Conference
dc.identifierhttps://arxiv.org/abs/astro-ph/0401335
dc.identifierhttp://arxiv.org/abs/astro-ph/0401335
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7266
dc.subjectAstrophysics
dc.titleThe Effect of aberration on polarization position angle of pulsars
dc.typetext

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