Fig. 4

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SEDs for the smooth-wind case for the (a) adiabatic (green) and (b) radiative (blue) regimes considering regions up to 1.5d from the star at inferior conjunction (INF; ϕ = 0.716) and superior conjunction (SUP; ϕ = 0.058). The synchrotron (colored dashed) and IC (colored solid) components are plotted, and the unabsorbed spectra (colored dotted) are also shown for comparison. As a reference, the shaded areas indicate the synchrotron (~10–2 eV) and IC (~107 eV) photon energies corresponding to the (adiabatic-to-radiative) transition particle energy for all individual emitters in the CD.
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