arXiv (OAI Expanded)
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Energy-Resolved Limits on Orbital X-ray Polarization Modulation in Cygnus X-1
Reflection off the companion star and its focused stellar wind is predicted to modulate the X-ray polarization of black hole X-ray binaries at half the orbital period ($P_{\rm orb}/2$), with an energy-dependent amplitude. We test this prediction against all publicly available IXPE observations of Cy
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