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Please use this identifier to cite or link to this item: http://localhost:80/xmlui/handle/123456789/1539
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dc.contributor.authorQadir, A-
dc.contributor.authorRafique, M-
dc.date.accessioned2019-11-19T10:04:52Z-
dc.date.available2019-11-19T10:04:52Z-
dc.date.issued1986-01-01-
dc.identifier.issn3 189-
dc.identifier.urihttp://142.54.178.187:9060/xmlui/handle/123456789/1539-
dc.description.abstractA formula is provided to check the correlation of pulsars and supernova remnants, using only observable pulsar parameters. The validity of this formula depends on the assumption that the value of the initial pulsar frequency is much greater than the present value. A test for this assumption is suggested.en_US
dc.language.isoen_USen_US
dc.subjectNatural Scienceen_US
dc.subjectPulsar supernovaen_US
dc.subjectremnant correlationen_US
dc.titlePulsar supernova remnant correlationen_US
dc.typeArticleen_US
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