Fig. 1

Effelsberg Stokes I map at λ 3.6 cm of NGC 4631 with apparent magnetic field orientation. The length of the vectors is proportional to the polarized intensity (1″ Ӕ 41μJy/beam). The colorscale gives the flux density in mJy/beam. The angular resolution is 85″. The rms noise (σ) is of 350 μJy/beam. Contour levels correspond to σ·( − 3,3,6,12,24,48,96,192,384). The “ × ” pinpoints the dynamical center.
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