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Fig. 10
Ratio of the Ordered-to-turbulent magnetic field strengths Bord/Btur vs. star formation surface density ΣSFR in NGC 6946. The dashed line shows the corresponding fitted line in NGC 4254 shifted by 0.2 along the x-axis (y = −0.32 x − 0.7, see Fig. 7b in Chyży 2008).
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