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New strong non-spiralling-in gravitational wave (GW) source for LIGO/VIRGOdetectors are proposed. Double O-Ne-Mg white dwarf mergers can produce stronggravitational waves with frequencies in the several hundreds Hz range. Suchevents can be followed by a Super Nova type Ia.

Double O-Ne-Mg white dwarfs merging as the source of the Powerfull Gravitational Waves for LIGO/VIRGO type interferometers