Fig. 3.
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Spectral energy distribution of a single blackbody component with a luminosity corresponding to the disk luminosity of Ton 599 and temperatures of 1200 K (blue) and 1500 K (orange) along with a model for a torus including an outflowing wind from Hönig & Kishimoto (2017, black). The observed value for the compact emission in our GRAVITY data is shown by the red symbol.
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