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We consider the possibility of observing supernova (SN) - gamma-ray burst(GRB) pairs separated by several years. These energetic events correspond tothe second SN explosion in a double star system followed by the formation ofthe very short-lived pair of compact objects and finally by the GRB generationafter their merge. Possible connection of SN 1997ds and GRB 990425 isdiscussed.

Can the same generation of astronomers see both the short gamma-ray bursts and their supernovae precursors?