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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2108
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dc.contributor.authorKonar, S-
dc.date.accessioned2008-03-03T10:02:27Z-
dc.date.available2008-03-03T10:02:27Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 299 - 301en
dc.identifier.urihttp://hdl.handle.net/2248/2108-
dc.description.abstractIt has been argued that some of the pulsars could be strange stars because these too are capable of supporting fast rotations observed in pulsars. We examine this claim from the point of view of the evolution of magnetic field in pulsars and find that there is no compelling reason for the existence of strange pulsars.en
dc.format.extent188872 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..299Ken
dc.subjectMagnetic fieldsen
dc.subjectStars-neutronen
dc.subjectStars-strangeen
dc.subjectPulsars-generalen
dc.titleWhither strange pulsars?en
dc.typeArticleen
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