Fig. A.10.
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3D-BAROLO modeling results for IRAS 04296+2923 (panels a and b) and H I 0432+2926 (panels c and d), based on the VLA D- and C-configuration H I data. For each subpanel, the columns show (from left to right) the observed data, the best-fit model, and the residuals for the integrated intensity (top row), velocity field (middle row), and velocity dispersion (bottom row).
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