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 [ ] 10.1086/303752, https://ui.adsabs.harvard.edu/abs/1997ApJ...477..897B 477
1 Pith paper cite this work, alongside 81 external citations. Polarity classification is still indexing.
1
Pith paper citing it
81
external citations · OpenAlex
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.