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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4974
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dc.contributor.authorAsgekar, Ashish-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2012-07-17T04:49:05Z-
dc.date.available2012-07-17T04:49:05Z-
dc.date.issued2001-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2001, Vol.326, p1249en
dc.identifier.issn0035-8711-
dc.identifier.issn1365-2966 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4974-
dc.descriptionRestricted Access.en
dc.description.abstractIn the previous paper of this series, Deshpande & Rankin reported results regarding the sub-pulse drift phenomenon in pulsar B0943+10 at 430 and 111MHz. This study has led to the identification of a stable system of sub-beams circulating around the magnetic axis of this star. Here, we present a single-pulse analysis of our observations of this pulsar at 35MHz. The fluctuation properties seen at this low frequency, as well as our independent estimates of the number of sub-beams required and their circulation time, agree remarkably well with the reported behaviour at higher frequencies. We use the `cartographic' transform mapping technique developed by Deshpande & Rankin in Paper I to study the emission pattern in the polar region of this pulsar. The significance of our results in the context of radio emission mechanisms is also discussed.en
dc.language.isoenen
dc.publisherWiley Balckwellen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001MNRAS.326.1249Aen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0110142en
dc.relation.urihttp://dx.doi.org/ 10.1111/j.1365-8711.2001.04664.xen
dc.rights2001 Royal Astronomical Societyen
dc.subjectradiation mechanismsen
dc.subjectnon-thermal; pulsarsen
dc.subjectgeneral; pulsarsen
dc.subjectindividual: B0943+10en
dc.titleThe topology and polarization of sub-beams associated with the `drifting' sub-pulse emission of pulsar B0943+10 - II. Analysis of Gauribidanur 35-MHz observationsen
dc.typeArticleen
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