Fig. 19.
Different components used in star formation estimates. Following Leroy et al. (2008) and Ford et al. (2013), we subtract the stellar component on the 24 μm Spitzer map (left panel) and on FUV GALEX map (right panel). The positions of the IRAM-PdB interferometer CO(1-0) observations are shown with white dashed circles. The yellow contour corresponds to the FUV flux (non-corrected for Galactic extinction) of 0.09 MJyr sr−1.
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