Accreting X-ray pulsars are predicted to produce detectable gamma-ray lines at 2.2-67.5 MeV plus a 511 keV annihilation line, with observability limited by magnetospheric absorption and radiative deceleration.
@doi [ ] 10.1093/mnras/235.1.51, https://ui.adsabs.harvard.edu/abs/1988MNRAS.235...51B 235
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Gamma-ray lines, electron-positron annihilation, and possible radio emission in X-ray pulsars
Accreting X-ray pulsars are predicted to produce detectable gamma-ray lines at 2.2-67.5 MeV plus a 511 keV annihilation line, with observability limited by magnetospheric absorption and radiative deceleration.