Local H I filaments driven by a small-scale dynamo - Unraveling the velocities and tangling of dusty magnetized structures

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Fig. 7

Orientation angles according to Eq. (3). Top: from the FIR distribution at 857 GHz.Middle: from the best fit H I distribution. Bottom: distribution of orientation angles according to Eq. (4) calculated from Stokes parameters U and Q of the 353 GHz FIR distribution.

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