Fig. 8.
Various physical maps of a face-on view of M 51. Top row, from left to right: SFR, stellar mass, and specific star formation rate spatial maps. Bottom row, from left to right: dust temperature, dust mass, and dust density spatial maps. All maps, except the dust temperature map, are in log-scale. All maps share the same pixel scale as the PACS 160 μm image: 4.0″.
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