| 1. The mass of the central black hole engine |
| 2. The rate of mass accretion |
| 3. The angular momentum of the central source (its magnitude and its orientation relative to the observer) |
The significance of the magnitude of the angular momentum is twofold. First, the orbital motion of charged particles around the black hole determines whether electromagnetic effects are large enough to form and collimate relativistic jets of particles. High velocity revolution of plasma would increase the electromagnetic effects and make jets more likely. Second, if jets are formed, rapid rotation of the black hole engine leads to a gyroscopic stabilizing force that keeps the jets pointed in the same direction. (Since some jets are nearly straight over distances of millions of light years, the direction that the jet source points must be almost constant for millions of years.)
Although these are plausible ideas, we stress that it is not yet certain that the understanding of jets and whether AGNs are radio loud can be reduced to such simple terms.