SummaryPreliminary attempts to observe 13 bright southern galaxies are described. Of these 10 were detected, including the Magellanic Clouds. The latter were studied in detail. Supplementary measurements on the Milky Way near the galactic centre were made and also some unsuccessful attempts to observe two globular clusters. Taking these results in conjunction with some observations of Brown and Hazard it is possible to derive a consistent picture of the radio emitting properties of " normal" galaxies.It is found that radio emission probably occurs with two markedly different distributions, one displaying characteristics of a type I population, the other having a very extensive, roughly spherical, spatial distribution quite unlike any known stellar population. Both distributions have a non-thermal spectrum, and the relative contributions of each appear to vary between different galaxy types. In general terms, although not altogether in detail, these results support the conclusions reached by Shklovskii concerning the distribution of radio emission in the Galaxy; also his interpretation of the spherical distribution as the result of relativistic electrons radiating in weak magnetic fields is examined, and found, with some modifications, to afford a plausible explanation of the observed differences between the radiating efficiencies of different types of galaxies.