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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2452
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dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorSrinivasan, G.-
dc.date.accessioned2007-05-25T09:22:57Z-
dc.date.available2007-05-25T09:22:57Z-
dc.date.issued1981-
dc.identifier.citationIAU Symposium, 1981, Vol.95, p417en
dc.identifier.urihttp://hdl.handle.net/2289/2452-
dc.descriptionOpen Access. Pulsars: 13 years of research on neutron stars; Proceedings of the Symposium, Bonn, West Germany, August 26-29, 1980. (A82-32926 15-90) Dordrecht, D. Reidel Publishing Co., 1981.en
dc.description.abstractThe recently introduced concept of a window of magnetic field strengths in which pulsars can be active is used to explain the variation in morphology of supernova remnants. Neutron stars created with field strengths of a value permitting pulsar activity result in particle production and Crab-like, centrally-concentrated remnants. Other field values lead to strong magnetic dipole radiation and consequent shell formation, e.g., Cas A.en
dc.format.extent203357 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherReidelen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1981IAUS...95..417Ren
dc.rights1981 Reidelen
dc.subjectPulsarsen
dc.subjectStellar magnetic fieldsen
dc.subjectStellar radiationen
dc.subjectStellar structureen
dc.subjectSupernova Remnantsen
dc.subjectMagnetic dipolesen
dc.subjectMagnetic fluxen
dc.subjectMilky way galaxyen
dc.subjectNeutron starsen
dc.subjectParticle productionen
dc.subjectStellar evolutionen
dc.titlePulsar activity and supernova remnant morphologyen
dc.typeArticleen
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