Fig. 12.
Left: modelled radial profiles of total radio emission of an M 51-like galaxy seen face-on at 30, 150, and 1400 MHz. Middle: model vertical profiles of total radio emission of an M 51-like galaxy seen edge-on at 30, 150, and 1400 MHz. Right: local synchrotron spectra of the galaxy at different distances along the galaxy major axis from the centre.
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