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Please use this identifier to cite or link to this item: http://localhost:80/xmlui/handle/123456789/1469
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dc.contributor.authorAsghar, Qadir-
dc.contributor.authorRafique, M-
dc.contributor.authorSiddiqui, A W-
dc.date.accessioned2019-11-18T10:15:03Z-
dc.date.available2019-11-18T10:15:03Z-
dc.date.issued1987-01-01-
dc.identifier.issn4 177-
dc.identifier.urihttp://142.54.178.187:9060/xmlui/handle/123456789/1469-
dc.description.abstractThe relativistic explanation of pulsar drift is based on an extremely simplistic model. The collapsing star is treated as composed of a collection of particles falling radially inwards. A calculation incorporating a finite angular momentum is found to give reasonable drift velocities provided the initial pulsar frequency is sufficiently high. The values required are not unreasonable.en_US
dc.language.isoen_USen_US
dc.publisherInstitute of Physics (IOP)en_US
dc.subjectNatural Scienceen_US
dc.subjectPulsar driften_US
dc.subjectrotational collapseen_US
dc.titlePulsar drift and rotational collapseen_US
dc.typeArticleen_US
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