volume 13, issue S337, P237-240 2017
DOI: 10.1017/s1743921317009498
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Abstract: AbstractThis talk commented on our progress in understanding high Ė pulsar output, with the photon power dominated by GeV radiation and the total power dominated by the e±/B wind. We are increasingly appreciating the anisotropy in these outflows, with high energy pulsar beaming probed by the distribution of γ-ray pulse profiles and wind anisotropy mapped by synchrotron images of PWNe. Possible hemispheric asymmetry and the prospects for additional probes of pulsar spindown, particularly from compact binaries i…

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