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Polarized X-Rays from Windy Accretion in Cygnus X-1

  • Authors: Juri Poutanen, Alexandra Veledina, Andrei M. Beloborodov

Juri Poutanen et al 2023 The Astrophysical Journal Letters 949 .

  • Provider: AAS Journals

Caption: Figure 3.

Energy dependence of the PD for the three models shown in Figure 2. The blue and red lines correspond to the inclinations of 30° and 60°, respectively. Solid, dotted, dashed, and dotted–dashed lines correspond to the outflow velocities of β 0 = 0, 0.2, 0.4, and 0.6, respectively. In the middle panel, the red curves for β 0 = 0.4 and 0.6 coincide.

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