Fig. 8.
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MOKA3D rotating disk best-fit model of J0957−2242 traced by the [O III]5007 transition. Panels show the observed (top), best-fit (center), and residual (bottom) moment maps. The residual maps were obtained by subtracting the model from the observed moment maps. The star marks the kinematic center, inferred as the peak flux emission. Pixels are masked at SN ≤ 4.
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