2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/35128Inspiraling compact binaries are expected to be the strongest sources of gravitational waves for VIRGO, LIGO and other laser interferometers. We present the first computations of quasi-equilibrium sequences of compact binaries containing two strange quark stars (which are currently considered as a possible alternative to neutron stars). We study a precoalescing stage in the conformal flatness approximation of general relativity using a multidomain spectral method. A hydrodynamical treatment is performed under the assumption that the flow is irrotational.4 pages, 2 PostScript figures, to appear in the Proceedings of the SF2A 04, Paris, FranceGeneral Relativity and Quantum CosmologyQuasiequilibrium sequences of binary strange quark stars in general relativitytext