Fig. 5.
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Moment 1 and moment 2 maps for the component of the [OIII]λ5007 line emission tracing gas in the host galaxy (see text). The contours are the same as in Fig. 4. An S/N > 40 threshold has been used to mask lower S/N spaxels and isolate the rotation in the central spaxels. A rotational pattern is suggested by the data that is compatible with the CO(5−4) rotation detected by B18.
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