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Fig. 17
Model comparisons to the absolutely flux calibrated near-infrared spectrum of the T7.5 dwarf Gliese 570 D (Burgasser et al. 2000). Three models are shown all calculated self-consistently using Kresonance line broadening from BV03 (top), A07 (middle), and A16 (bottom), for Teff = 800 K, log (g) = 5.0, and R∕R⊙ = 0.082.
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