Pulsar supernova remnant correlation

dc.contributor.author	Qadir, A
dc.contributor.author	Rafique, M
dc.date.accessioned	2019-11-19T10:04:52Z
dc.date.available	2019-11-19T10:04:52Z
dc.date.issued	1986-01-01
dc.identifier.issn	3 189
dc.identifier.uri	http://142.54.178.187:9060/xmlui/handle/123456789/1539
dc.description.abstract	A 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.iso	en_US	en_US
dc.subject	Natural Science	en_US
dc.subject	Pulsar supernova	en_US
dc.subject	remnant correlation	en_US
dc.title	Pulsar supernova remnant correlation	en_US
dc.type	Article	en_US