Abstract
A recent model1 for the 1011–1015 eV γ-ray emission from the 1.24-s X-ray pulsar Hercules X-l postulates coherent charged particle beams as the photon source, through a cascade process in intervening matter in the binary system HZ Her/Her X-1. This interpretation is complicated by a 1985 observation2 of ∼1012-eV γ-ray pulsations during at least the first hour of the nominal 6-h X-ray eclipse of Her X-1 by HZ Her, which would completely absorb a particle (or photon) beam propagating along or near the line of sight to Her X-1. Here we show that the presence of even a weak dipole magnetic field around the companion star is sufficient to steer such a beam to a suitable target region for producing the observed γ-rays. We demonstrate that models such as that in ref. 1 must include such effects, and we discuss the effects of such beam steering on γ-ray and neutrino observations.
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Gorham, P., Learned, J. Companion-star beam steering of high-energy particles from Hercules X-1. Nature 323, 422–424 (1986). https://doi.org/10.1038/323422a0
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DOI: https://doi.org/10.1038/323422a0
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