Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7232
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dc.contributor.authorMcSweene, Samuel J.-
dc.contributor.authorBhat, N. D. Ramesh-
dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorTremblay, S.E.-
dc.date.accessioned2019-07-03T18:35:34Z-
dc.date.available2019-07-03T18:35:34Z-
dc.date.issued2017-09-
dc.identifier.citationProceedings of IAU Symposium 2017, Vol.13, p376-377en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2289/7232-
dc.descriptionRestricted Access.en_US
dc.description.abstractWe observed single pulses from PSR J0034-0721 (B0031-07) simultaneously at the MWA (185 MHz) and the GMRT (610 MHz). Correlation analyses reveal that the phase difference of the average profiles at the two frequencies differs from the phase difference observed between individual subpulses, indicating that the individual emission columns above the pulsar’s rotating carousel of sparks do not evolve in frequency in the same way that the global magnetosphere does. This hints at a possible departure from the dipolar field geometry in this pulsar’s emission region. Moreover, the discrepancy depends on the drift mode, suggestive of a way to constrain the emission heights associated with each drift mode.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.urihttp://adsabs.harvard.edu/doi/10.1017/S1743921317008420en_US
dc.relation.urihttps://doi.org/10.1017/S1743921317008420en_US
dc.rights2018 International Astronomical Unionen_US
dc.subjectPulsarsen_US
dc.subjectgeneralen_US
dc.subjectindividual (J0034-0721)en_US
dc.titlePhase shifts in multi-frequency observations of the drift bands of J0034-0721en_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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