Fig. 13.
Emergent spectra (top panel) and temperature structures (bottom panel) of the models with solar chemical abundance and three intrinsic luminosities, ℓ = 0.5, 0.1 and 0.001, but with the same parameters of the accreting particles (ℓa = 0.05, η = 0.75, χ = 0.2, Ψ = 60°). The spectrum and the temperature structure of the undisturbed models are also shown by the dashed curves.
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