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Fig. 2.

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Characterisation of the star-forming knots in the stripped material of NGC 3314A in the MUSE FoV. Left: knots colour-coded by their emission-line ratios on the kernel-smoothed Hα map. In both panels, the point circled in red denotes a knot whose spectrum is likely contaminated by a background galaxy (appearing as a black feature on the kernel-smoothed Hα map). Right: BPT diagram of knots in the stripped arms of NGC 3314A with the same colour code. The orange line denotes the theoretical demarcation between starbursts and galaxies hosting active galactic nuclei (Kewley et al. 2001).

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