Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7890
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dc.contributor.authorMaan, Yogesh-
dc.contributor.authorAswathappa, H.A.-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2022-02-10T08:51:59Z-
dc.date.available2022-02-10T08:51:59Z-
dc.date.issued2012-09-01-
dc.identifier.citationMonthly Notices of Royal Astronomical Society, 2012, Vol. 425, p2-7en_US
dc.identifier.issn0035-8711-
dc.identifier.issn1365-2966 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/7890-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractWe report our search for and a possible detection of periodic radio pulses at 34.5 MHz from the Fermi Large Area Telescope pulsar J1732-3131. The candidate detection has been possible in only one of the many sessions of observations made with the low-frequency array at Gauribidanur, India, when the otherwise radio weak pulsar may have apparently brightened many folds. The candidate dispersion measure along the sight line, based on the broad periodic profiles from ∼20 min of data, is estimated to be 15.44 ± 0.32 pc cc-1. We present the details of our periodic and single-pulse search, and discuss the results and their implications relevant to both, the pulsar and the intervening medium.en_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2012MNRAS.425....2M/abstracten_US
dc.relation.urihttps://arxiv.org/abs/1109.6032en_US
dc.relation.urihttps://doi.org/10.1111/j.1365-2966.2012.20608.xen_US
dc.rights2012 The Author(s)en_US
dc.subjectstars: neutronen_US
dc.subjectpulsars: generalen_US
dc.subjectpulsars: individualen_US
dc.subjectgamma-raysen_US
dc.subjectradio continuumen_US
dc.subjectAstrophysics of Galaxiesen_US
dc.subjectHigh Energy Astrophysical Phenomenaen_US
dc.titlePulsed radio emission from the Fermi-LAT pulsar J1732-3131 : search and a possible detection at 34.5 MHzen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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