Fig. 1

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Images of the jet in Hα and [S II]λ6731, with the prominent HH objects labelled. The image corresponds to a ~12.5 Å wide spectral bin centred on the peak of the emissions. It is rotated by an angle of 47.3° with respect to the plane of the sky. We note the lack of emission in the first few arcseconds due to the saturation effects discussed in Sect. 2.
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