2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/13024Hydrodynamic simulations were performed of the dynamical phase of the merging of binary neutron stars (NS-NS) and of neutron star black hole binaries (NS-BH), using the physical nuclear equation of state of Lattimer and Swesty (1991) and taking into account the emission of gravitational waves and neutrinos.4 pages, 4 ps figures, submitted to Editions Frontieres (France), Nuclei in the Cosmos VAstrophysicstext