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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2795
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dc.contributor.authorKonar, S-
dc.contributor.authorChoudhuri, A. R-
dc.date.accessioned2008-07-22T07:53:08Z-
dc.date.available2008-07-22T07:53:08Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 697 - 698en
dc.identifier.urihttp://hdl.handle.net/2248/2795-
dc.description.abstractA possible mechanism for screening of the surface magnetic field of an accreting neutron star, by the accreted material, is investigated. In particular, we investigate the nature of the evolution of the internal field configuration in the case of a) a polar cap accretion and b) spherical accretion.en
dc.format.extent81195 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectMagnetic Fieldsen
dc.subjectNeutron Starsen
dc.subjectAccretion-Material Flowen
dc.titleDiamagnetic screening of the magnetic field in accreting neutron starsen
dc.typeArticleen
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