Fig. 9
Contours and apparent B-vectors (not corrected for Faraday rotation) of polarized intensity of NGC 2976 from the WSRT-SINGS data superimposed on the DSS blue image. The contour levels are (3, 5, 8, 16, 32, 64) × 25 (rms noise level) μJy/beam. The vector of 10′′ length corresponds to the polarized intensity of about 31.3 μJy/beam. The map resolution is 48.6′′× 45.0′′ HPBW.
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