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    Modelling energy-dependent pulsar light curves

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    Date
    2018
    Author
    Venter, Christo
    Barnard, Monica
    Harding, Alice K.
    Kalapotharakos, Constantinos
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    Abstract
    In 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 cyl
    URI
    http://hdl.handle.net/10394/31492
    https://doi.org/10.1017/S1743921317008493
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    • Conference Papers - Potchefstroom Campus [713]
    • Faculty of Natural and Agricultural Sciences [4855]

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