Fig. B.1.
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[O III]λ5007 velocity field (km s−1), velocity dispersion (km s−1), and flux intensity (erg s−1 cm−2) maps for the narrow component. The maps are as in the lower panel of Fig. 5, and are included here as reference. The black solid line indicates the major axis of the stellar rotation (Table 4). The dashed lines indicate the orientation of the radio jet (Table 1).
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