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Fig. A.13
Finding charts for the stars and filaments Paumard et al. (2006), Viehmann et al. (2006), Mužić et al. (2007) mentioned in this work, demonstrated for the inner 10′′ (0.4 pc) on a NIR L’ (3.8 μm) emission image (Sabha, priv. comm., here: arbitrary units).
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