Magnetic fields and cosmic rays in M 31 - II. Strength and distribution of the magnetic field components

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Fig. 7.

Variations in the strengths of the equipartition and non-equipartition total fields at $1 \overset{'}{.} 5$ $1{{\overset{\prime}{.}}}5$ resolution with azimuthal angle in the galaxy plane, counted from the north-eastern major axis in the sky plane (left side in Fig. 6), averaged in 10°–sectors of the radial ring 8–12 kpc.

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