A Model for Simulating Realistic Profiles of Pulsars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5587

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DC Field	Value	Language
dc.contributor.author	Thomas, R. M. C	-
dc.contributor.author	Gupta, Y	-
dc.contributor.author	Gangadhara, R. T	-
dc.date.accessioned	2011-09-28T09:13:45Z	-
dc.date.available	2011-09-28T09:13:45Z	-
dc.date.issued	2011-08	-
dc.identifier.citation	AIP Conference Proceedings, Vol. 1357, pp. 297-298	en
dc.identifier.uri	http://hdl.handle.net/2248/5587	-
dc.description	Restricted Access	en
dc.description.abstract	We devise an accurate method to compute the emission profile corresponding to a given set of pulsar emission parameters, for eg. inclination angle alpha, impact angle beta, frequency of emission omega, Lorentz factor gamma, and pulsar spin-period P. The intensity of emission is simulated, and compared with the observed profiles	en
dc.language.iso	en	en
dc.publisher	American Institute of Physics	en
dc.relation.uri	http://link.aip.org/link/?APCPCS/1357/297/1	en
dc.rights	© American Institute of Physics	en
dc.subject	Pulsar	en
dc.subject	Geometry	en
dc.subject	Rotation	en
dc.title	A Model for Simulating Realistic Profiles of Pulsars	en
dc.type	Article	en
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