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Fig. 15

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Relative orientation of the gas velocity and magnetic fields as a function of Ek/EB averaged over 20 pc cubical bins. The green distribution in the background includes only gas in the CMZ and excludes the gas in the bar lanes. The black lines show the average (solid) and median (dotted) of the distribution. Once the turbulence becomes dynamically important, the relative orientation becomes more random. An exception is given by gas in the dust lanes, for which the average (solid grey line) and median (dotted grey line) are shown.

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