Fig. 1
MUSE observation of Th 28, showing the jet in the combined Hα emission across all velocities before continuum subtraction. The positions of the star (black cross) and all knots discussed in this paper are indicated. A number of background stars are visible in the field, as is the western Herbig Haro object associated with the red-shifted jet. The estimated FWHM of the PSF is 0′′. 9–1′′.
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