The radio continuum structure of bright galaxies at 1.4 GHZ.

The (double) source structure of the radio continuum emission of the more powerful radio sources associated with galaxies is only briefly discussed in Chapter VI. In Chapter VII we gave a fractional luminosity function for these sources. Some evidence is presented that it is not the lack of gas in elliptical and lenticular galaxies which causes the occurrence of the double source structure in these galaxies. The results indicate that the mass of an elliptical or of the bulge component of a lenticular determine whether these galaxies manage to have strong radio continuum emission with a double lobed structure... Zie: Summary