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dc.contributor.author Panchapakesan, N
dc.date.accessioned 2008-05-27T12:15:25Z
dc.date.available 2008-05-27T12:15:25Z
dc.date.issued 2003
dc.identifier.citation BASI, Vol. 31, No. 3&4, pp. 195 - 199 en
dc.identifier.uri http://hdl.handle.net/2248/2364
dc.description.abstract Magnetars 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.extent 151187 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2003BASI...31..195P en
dc.subject Neutron stars en
dc.subject High magnetic fields en
dc.subject Magnetars en
dc.title Magnetars- A Review en
dc.type Article en


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