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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2363
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dc.contributor.authorKonar, S-
dc.date.accessioned2008-05-27T12:06:42Z-
dc.date.available2008-05-27T12:06:42Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 187 - 193en
dc.identifier.urihttp://hdl.handle.net/2248/2363-
dc.description.abstractThere has been strong observational evidence suggesting a casual connection between the binary history of neutron stars and the evolution of their magnetic field. In this article we discuss one of 3 the plausible mechanisms proposed for the evolution of the surface magnetic field, that of the diamagnetic screening of the field by accreted material.en
dc.format.extent224124 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..187Ken
dc.subjectMagnetic fieldsen
dc.subjectNeutron starsen
dc.subjectAccretion-material flowen
dc.titleThe Binary History and the Magnetic Field of Neutron Starsen
dc.typeArticleen
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