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Fig. 3.

image

Atmosphere structure (left) and the spectrum of the escaping radiation (right) for mono-energetic return current. Left panels: dependence of the electron number density ne, energy loss of the return current mQ+, and the temperature T on the column density. The red curves correspond to a model with Lorentz factor γ0 = 500, the blue curves are for γ0 = 50, and the black curves are for γ0 = 10. The parameters are Teff, h = 5 MK, Teff, i = 1.6 MK, and log g = 14.3. The corresponding structure and the spectrum for model without external heating (Teff, i = 5 MK, Teff, h = 0) are shown with the magenta dashed curve.

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