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 |