We review the current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries. First. procedures for a solution of BH-NS binaries in quasi-equilibrium circular orbits and the numerical results. such as quasi-equilibrium sequence and mass-shedding limit. https://www.pomyslnaszycie.com/white-and-green-bulletin-board-border-simply-boho-schoolgirl-style-on-sale/