Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/5587
Title: | A Model for Simulating Realistic Profiles of Pulsars |
Authors: | Thomas, R. M. C Gupta, Y Gangadhara, R. T |
Keywords: | Pulsar Geometry Rotation |
Issue Date: | Aug-2011 |
Publisher: | American Institute of Physics |
Citation: | AIP Conference Proceedings, Vol. 1357, pp. 297-298 |
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 |
Description: | Restricted Access |
URI: | http://hdl.handle.net/2248/5587 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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A Model for Simulating Realistic Profiles of Pulsars.pdf Restricted Access | Restricted Access | 821.37 kB | Adobe PDF | View/Open Request a copy |
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