Blazars, Gamma Ray Bursts and Galactic superluminal sources
  BeppoSAX is best known for its role in the disclosure of the Gamma-Ray Burst mystery, but it has also improved our understanding of jetted sources in general, and blazars in particular. On the interpretational side, we are curious to see if all sources with relativistic jets (or "flying pancakes", as in GRBs) are controlled by the same basic physics, despite the very different lifetimes and behavior. To this end we explore some general characteristics of blazars, GRBs and superluminal galactic sources, such as their bulk Lorentz factors, the power of their jets compared with what they can extract through accretion, and the value of the magnetic field, close to the black hole, needed to extract the spin energy of a rotating black hole. We find remarkable similarities, namely that the outflowing mass rate is of the order of 1 per cent of the accretion mass rate in all systems, and that the value of the magnetic field required to efficiently extract the spin energy of the black hole is of the order of the gravitational energy density of the matter close to the gravitational radius. We then go on to discuss the way in which the energy in bulk relativistic motion can be transformed into beamed radiation, and consider the possibility that all three classes of sources could work in the same way, namely by a intermittent release of relativistic plasma at the base of the jet and thus with similar efficiency. Different patches of material, with slightly different velocities, collide at some distance from the black hole, producing the radiation we see. 
G. Ghisellini (Osserv. Astr. di Brera, Merate, Italy) and A. Celotti   (Sissa, Trieste, Italy)