Fig. B.3
Left: observation of GG Tau A in near-infrared (H-Band) with Gemini/Hokupa’a (Credit: Daniel Potter/University of Hawaii Adaptive Optics Group/Gemini Observatory/AURA/NSF). Right: intensity maps of GG Tau A that are simulated at λ = 1.65 μm. The images are convolved with a Gaussian beam of 0.05′′ × 0.05′′ to take the resolution of the Gemini/Hokupa’a telescope into account. The model consists of disks around Aa and Ab1 in the same plane as the circumbinary disk and a disk around Ab2 that is inclined by 90 ° with a position angle of the rotation axis of 270° (see Fig. 2).
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