Fig. 1
Contours of the total power radio continuum of NGC 4254. The radio image at 4.86 GHz with a resolution of 15″ and B-vectors proportional to the polarized emission (Chyży et al. 2007) is overlaid on the XMM-Newton Optical Monitor UVW2 filter image. The contours are at: 3, 8, 16, 32, 64, 128, 230, and 350 × 10 μJy/beam area. Vectors of length of 1″ correspond to a polarized intensity of 10 μJy/beam area. The beam size is shown in the lower left corner of the figure.
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