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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3886
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dc.contributor.authorKapoor, R. C-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-09-24T14:49:45Z-
dc.date.available2008-09-24T14:49:45Z-
dc.date.issued1986-12-
dc.identifier.citationAstrophysical Journal, Part 1 , Vol. 311, No. 2, pp. 680 - 683en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/3886-
dc.description.abstractGeneral relativistic effects due to spacetime curvature and rotation on the arrival times of pulsar signals are investigated using a rotationally perturbed spherical metric. It is found that for the millisecond pulsar PSR 1937+214, the advancement in arrival time (assuming the usual polar cap model for emission mechanism and a radius-to-frequency mapping) due to these effects is nontrivial. The results are compared with recent multifrequency timing measurements on PSR 1937+214, and the implications regarding emission region thickness and emission mechanism for fast pulsars are pointed out.en
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1986ApJ...311..680Ken
dc.subjectPulsarsen
dc.subjectPulse rateen
dc.subjectRelativistic effectsen
dc.subjectSignal analysisen
dc.subjectSpace-time functionsen
dc.subjectDragen
dc.subjectPolar capsen
dc.subjectStellar modelsen
dc.subjectStellar rotationen
dc.titleEffects of spacetime curvature and rotation on arrival times of pulses from fast pulsarsen
dc.typeArticleen
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