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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2793
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dc.contributor.authorJoshi, B. C-
dc.contributor.authorLyne, A. G-
dc.contributor.authorJordan, C-
dc.contributor.authorKrawczyk, A-
dc.contributor.authorGil, J. A-
dc.date.accessioned2008-07-22T07:21:19Z-
dc.date.available2008-07-22T07:21:19Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 691 - 693en
dc.identifier.urihttp://hdl.handle.net/2248/2793-
dc.description.abstractTwo kinds of irregularities are observed in the rotation rates of pulsars - timing noise and glitches. A study of these irregularities is useful as a probe for the internal structure of these stars. We present the distribution of fractional change in the rotation rate of pulsars as obtained from all available data.en
dc.format.extent71283 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectRadio Pulsarsen
dc.subjectPulsars-Timong Noise and Glitchesen
dc.titleObservations of rotational instabilities in Radio Pulsarsen
dc.typeArticleen
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