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dc.contributor.authorVenter, Christo
dc.contributor.authorBarnard, Monica
dc.contributor.authorHarding, Alice K.
dc.contributor.authorKalapotharakos, Constantinos
dc.date.accessioned2018-10-24T08:55:52Z
dc.date.available2018-10-24T08:55:52Z
dc.date.issued2017
dc.identifier.citationVenter, C. et al. 2017. Modelling energy-dependent pulsar light curves. (In Weltevrede, P., Perera, B.B.P., Preston, L.L. & Sanidas, S., eds. Pulsar astrophysics the next fifty years. Proceedings IAU Symposium No. 337, 2017). Proceedings of the International Astronomical Union, 13(S337):120-123. [https://doi.org/0.1017/S1743921317008493]en_US
dc.identifier.issn1743-9213
dc.identifier.issn1743-9221 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/31492
dc.identifier.urihttps://doi.org/0.1017/S1743921317008493
dc.description.abstractIn recent years, surprise discoveries of pulsed emission from the Crab and Vela pulsars above 100 GeV have drawn renewed attention to this largely unexplored region of the energy range. In this paper, we discuss example light curves due to curvature emission, with good resolution in the different energy bands. Continued light curve modelling may help to discriminate between different emission mechanisms, as well as constrain the location where emission is produced within the pulsar magnetosphere, including regions beyond the light cylen_US
dc.language.isoenen_US
dc.publisherCambridge Univ Pressen_US
dc.subjectGamma rays: theoryen_US
dc.subjectRadiation mechanisms: radiation mechanisms: nonthermalen_US
dc.subjectStars: magnetic fieldsen_US
dc.subjectStars: neutronen_US
dc.subject(Stars:) pulsars: individual (PSR B0531+21, PSR B0833-45)en_US
dc.titleModelling energy-dependent pulsar light curvesen_US
dc.typePresentationen_US
dc.contributor.researchID12006653 - Venter, Christo
dc.contributor.researchID20574266 - Barnard, Monica


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