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Please use this identifier to cite or link to this item: http://142.54.178.187:9060/xmlui/handle/123456789/1469
Title: Pulsar drift and rotational collapse
Authors: Asghar, Qadir
Rafique, M
Siddiqui, A W
Keywords: Natural Science
Pulsar drift
rotational collapse
Issue Date: 1-Jan-1987
Publisher: Institute of Physics (IOP)
Abstract: The 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.
URI: http://142.54.178.187:9060/xmlui/handle/123456789/1469
ISSN: 4 177
Appears in Collections:Journals

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