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Fig. 8.


Maps across the FOV of the maximum blue- (left panel) and red-shifted (central panel) velocities for the [O III] best-fit line profile. In particular, the two panels show the differences between maximum velocities (V02 and V98) and stellar velocity (Vstar), as labelled, to reveal outflow signatures. In the V98 − Vstar map the shell region (S) associated with both receding and approaching high-v gas is shown. The right panel shows the [O III] velocity width W80.

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