Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1600
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dc.contributor.authorNarayan, R.-
dc.contributor.authorVivekanand, M.-
dc.date.accessioned2006-12-19T10:35:43Z-
dc.date.available2006-12-19T10:35:43Z-
dc.date.issued1982-09-
dc.identifier.citationAstronomy and Astrophysics, 1982, Vol.113, pL3-L6.en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1600-
dc.description.abstractThe observed polarisation angle variation in pulsars is analysed on the basis of the magnetic pole model. The angles alpha between the rotation and magnetic axes and beta between magnetic axis and line of sight are estimated using (1) the shape of the polarisation angle (theta) vs pulse longitude (phi) curve, (2) the magnitude of the central gradient d theta/d phi in the main pulse, and (3) the magnitude and sign of the gradient in the interpulse. It is concluded that beta can have either sign, with outer lines of sight (i.e., away from the rotation axis) probably predominating. This result is contrary to certain theories which predict a complete absence of outer lines of sight. It is also concluded that alpha is not randomly distributed; small angles seem to be preferred.en
dc.format.extent566732 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1982A&A...113L...3Nen
dc.rights(1982) by the European Southern Observatory. Scanned images provided by the NASA ADS.en
dc.subjectBeams(radiation)en
dc.subjectGeometrical opticsen
dc.subjectPulsarsen
dc.subjectRadio astronomyen
dc.subjectStellar modelsen
dc.subjectAngles(geometry)en
dc.subjectAxes of rotationen
dc.subjectLine sighten
dc.subjectMagnetic polesen
dc.subjectPolarization characteristicsen
dc.subjectPolarized radiationen
dc.titleGeometry of pulsar beams - Relative orientations of rotation axis, magnetic axis, and line of sighten
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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