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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2364
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dc.contributor.authorPanchapakesan, N-
dc.date.accessioned2008-05-27T12:15:25Z-
dc.date.available2008-05-27T12:15:25Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 195 - 199en
dc.identifier.urihttp://hdl.handle.net/2248/2364-
dc.description.abstractMagnetars are neutron stars in which a decaying high magnetic field is the source of energy production. The suggestion that magnetars are the dominant source of energy for soft gamma repeaters and anomalous x-ray pulsars is examined. Some questions that arise, because of the very high magnetic fields, are considered.en
dc.format.extent151187 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..195Pen
dc.subjectNeutron starsen
dc.subjectHigh magnetic fieldsen
dc.subjectMagnetarsen
dc.titleMagnetars- A Reviewen
dc.typeArticleen
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