Fig. A.2.
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Overlay of ALMA 3 mm continuum contours (in black) on the CO(1–0) line map. This highlights the compactness of the continuum emission compared to the line emission in both members of the IRAS 05054+1718 galaxy pair. Neither the continuum contours nor the CO(1–0) line map is corrected for the PB, to ease the visualisation of the companion galaxy NED02.
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