  The introduction of the three interpretational paradigms for Gamma-Ray Bursts
(GRBs) and recent progress in understanding the X- and gamma ray luminosity in
the afterglow allow us to make assessments about the astrophysical settings of
GRBs. In particular, we evidence the distinct possibility that some GRBs occur
in a binary system. This subclass of GRBs manifests itself in a "tryptich": one
component formed by the collapse of a massive star to a black hole, which
originates the GRB; a second component by a supernova and a third one by a
young neutron star born in the supernova event. Similarly, the understanding of
the physics of quantum relativistic processes during the gravitational collapse
makes possible precise predictions about the structure of short GRBs.
