Magnetic fields and star formation in low-mass Magellanic-type and peculiar galaxies

W. Jurusik; R. T. Drzazga; M. Jableka; K. T. Chyży; R. Beck; U. Klein; M. Weżgowiec

doi:10.1051/0004-6361/201323060

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Volume 567 (July 2014)

A&A, 567 (2014) A134

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Fig. 3

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Total-power contours of radio emission without nearby background sources for NGC 4605 at 4.85 GHz a) and NGC 5204 at 8.35 GHz b). The contour levels and other map parameters are the same as in Figs. 1 and 2. The positions of the subtracted background sources are marked by asterisks.

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