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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2421
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dc.contributor.authorMitra, D.-
dc.contributor.authorKonar, Sushan-
dc.contributor.authorBhattacharya, D.-
dc.contributor.authorHoensbroech, A.V.-
dc.contributor.authorSeiradakis, J.H.-
dc.contributor.authorWielebinski, R.-
dc.date.accessioned2007-05-25T08:38:51Z-
dc.date.available2007-05-25T08:38:51Z-
dc.date.issued2000-
dc.identifier.citationASP Conference Series, 2000, Vol.202, p265en
dc.identifier.urihttp://hdl.handle.net/2289/2421-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations. ulsar Astronomy - 2000 and Beyond, ASP Conference Series, Vol. 202; Proceedings of the 177th Colloquium of the IAU held in Bonn, Germany, 30 August - 3 September 1999. (San Francisco: ASP). Eds. M. Kramer, N. Wex, and N. Wielebinski, 2000.en
dc.description.abstractThe evolution of the multipolar structure of the magnetic field of isolated neutron stars is studied assuming the currents to be confined to the crust. Lower orders ($\le 25$) of multipole are seen to evolve in a manner similar to the dipole suggesting little or no evolution of the expected pulse shape. We also study the multifrequency polarization position angle traverse of PSR B0329+54 and find a significant frequency dependence above 2.7 GHz. We interpret this as an evidence of strong multipolar magnetic field present in the radio emission region.en
dc.format.extent85139 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2000ASPC..202..265Men
dc.relation.urihttp://arxiv.org/abs/astro-ph/9911085)en
dc.rights2000 Astronomical Society of the Pacificen
dc.titleEvolution of multipolar magnetic fields in isolated neutron stars and its effect on pulsar radio emissionen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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