Pulsar drift and rotational collapse

Please use this identifier to cite or link to this item: http://localhost:80/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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