Image Details
Caption: Figure 2.
Flux and polarization spectra for different scattering strengths compared to the unscattered case in a simplified setup with Bp = 5 × 1013 G, kT = 0.6 keV, R = 10 km, a hot spot at (θs, ϕs) = (65°, 30°), viewing angle θ = 25°, and varying ζ ≡ ξτ/β0 = 0.8, 2.5, and 7.0 (see Equations (2) and (16)). Left and middle: the relative O-mode and X-mode fluxes. Right: the corresponding linear polarization degree PL(ω) as a function of energy.
© 2026. The Author(s). Published by the American Astronomical Society.