The status of the Supernova/Gamma-Ray Burst connection is reviewed. There is clear evidence that long duration Gamma-ray Bursts are associated with broad-line SNe-Ib/c, although some new studies show that GRBs could be produced in tight binary systems which consist of a massive Wolf-Rayet star and a neutron star companion. Present estimates produce a ratio GRB/SNe-Ibc in the range ∼0.4%-3%.
