The Cambridge group showed that most of these radio sources must lie outside our galaxy (indeed many of them could be identified with other galaxies) and also that there were many more weak sources than strong ones.
剑桥小组表明,这些射电源中的大部分一定位于我们银河系之外(实际上,其中许多可以与其他星系识别),而且弱源比强源多得多。