Pulsar drift and rotational collapse

dc.contributor.author	Asghar, Qadir
dc.contributor.author	Rafique, M
dc.contributor.author	Siddiqui, A W
dc.date.accessioned	2019-11-18T10:15:03Z
dc.date.available	2019-11-18T10:15:03Z
dc.date.issued	1987-01-01
dc.identifier.issn	4 177
dc.identifier.uri	http://142.54.178.187:9060/xmlui/handle/123456789/1469
dc.description.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.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Institute of Physics (IOP)	en_US
dc.subject	Natural Science	en_US
dc.subject	Pulsar drift	en_US
dc.subject	rotational collapse	en_US
dc.title	Pulsar drift and rotational collapse	en_US
dc.type	Article	en_US