Fig. 8
Synchrotron-FIR correlation (q) overlaid with contours of the star formation traced by free-free emission with contour levels of 20, 50, 100, 200, 400 μJy/beam (top), the ordered magnetic field traced by the linearly polarized intensity PI with contour levels of 85, 120, 160 μJy/beam (middle) and the turbulent magnetic field (Isyn − PI/0.75) with contour levels of 0.3, 0.6, 1, 2, 25, 32 mJy/beam (bottom) in NGC 6946.
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