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Constraining the PeV Gamma-Ray Emission Zone of Cygnus X-3 with Contemporaneous GeV Timing and Spectral Observations

  • Authors: Xing-Fu Zhang, Ruo-Yu Liu, Dmitriy Khangulyan, Cui-Yuan Dai, Xiang-Yu Wang

Xing-Fu Zhang et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure C1.

Upper panel: evolution of the orbital phases corresponding to the maximum (solid line) and minimum (dashed line) EC scattering efficiency as functions of H/H0. The horizontal dotted lines mark the superior and inferior conjunction phases. Lower panel: phase offsets of the EC extrema relative to the conjunctions. The solid curve shows ﹩{\rm{\Delta }}\phi =1.0-{\phi }_{{\rm{\max }}}﹩, and the dashed curve shows ﹩{\rm{\Delta }}\phi =0.5-{\phi }_{{\rm{\min }}}﹩. As the emission zone moves inward (H/H0 ≪ 1), both offsets approach zero, indicating that a compact inner emitter naturally peaks closer to the conjunction phases.

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