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Recent measurements of the Chandra satellite have shown that a supermassiveblack hole of $M = 2.6 \times 10^{6} M_{\odot}$ is located in the GalacticCenter; it seems probable that, from other observations, this fact is common inthe majority of galaxies. On the other hand, GRB explosions are typicalphenomenon linked to the galactic dynamics. In the present paper we discuss thepossibility that GRBs are tidal disruption of stars by supermassive black holeslocated in the center of galaxies. This conjecture can be tested by agravitational wave detector of the class of AURIGA.Comment: 4 pages, 2 figures talk at Gamma Ray Burst Symposium - Santa Fe, New  Mexico (USA) September 8-12, 2003. There were added four new references and  the entrances of the two figures were written in a more clear wa

Gravitational Waves and GRBs from Tidal Disruption of Stars in the Center of Galaxies