Fig. 10.
Bottom left:SPIRE SSW12CO emission maps showing the nine spaxels involved in the analysis. Top left: hard (green) and soft (red) X-ray emission from Chandra from Marinucci et al. (2012) of the outflow observed in the central region (∼1′ × 1′) in NGC 4945. Middle:12CO/IR results obtained using SSW SPIRE data (19″ beam) numbered following the scheme shown in the bottom-left panel. Right:12CO/IR results normalized to the emission of the central spaxel (red square).
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