Fig. 20.
Star formation estimate derived the FUV and 24 μm components indicated in Fig. 19 (left panel) and the correlation factor between these two components (right panel). The positions of the IRAM-PdB interferometer CO(1-0) observations are shown with white dashed circles. The yellow contour corresponds to a FUV GALEX flux (non-corrected for Galactic extinction) of 0.09 MJy sr−1.
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