Please use this identifier to cite or link to this item:
http://142.54.178.187:9060/xmlui/handle/123456789/1539Full metadata record
| DC Field | Value | Language |
|---|---|---|
| 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 |
| Appears in Collections: | Journals | |
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