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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2797
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dc.contributor.authorAhuja, A. L-
dc.contributor.authorGupta, Y-
dc.contributor.authorKembhavi, A. K-
dc.contributor.authorKulkarni, V-
dc.date.accessioned2008-07-22T09:26:05Z-
dc.date.available2008-07-22T09:26:05Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 701 - 702en
dc.identifier.urihttp://hdl.handle.net/2248/2797-
dc.description.abstractWe present preliminary results from an ongoing program of accurate pulsar dispersion measure (DM) measurements using the GMRT. From simultaneous dual frequency observations, we are able to determine OMs to accuracies of 1 part in 104 and better. For 4 of the 12 pulsars studied, we find our mean DM value to be significantly different from the expected value. For most of the pulsars, we detect significant variations of the DM on time scales of weeks to months.en
dc.format.extent86302 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectPulsar Dispersion Measuresen
dc.subjectGMRTen
dc.titleTracking pulsar dispersion measures using the GMRTen
dc.typeArticleen
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