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Fig. 2.
GALEX FUV, IRAC 3.6 μm, WISE 22 μm, and SPIRE 350 μm images for NGC 4725, NGC 4736 (M 94), NGC 5055 (M 63), and NGC 5457 (M 101). All images are convolved to the same FWHM and are shown on a square root scale.
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