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Fig. 3
Model spectral energy distributions of specific intensities for the carbon atmospheres with log g = 14.3 and two Teff = 2 and 4 MK, computed for four angles, μ = cosθ = 0.9306 (solid curves), 0.67 (dashed curves), 0.33 (dotted curves), and 0.0694 (dash-dotted curves).
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