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The nucleosynthesis of heavy elements in the scenario for the evolution of aclose binary of neutron stars differing greatly in mass is considered. Incontrast to the scenario for the merger of two neutron stars of comparablemasses considered repeatedly in the literature, the evolution of such a binaryat the final stage consists in a rapid mass transfer to the more massive starand an explosive disruption of the low-mass component. We provide the detailsof the explosion and calculate the abundances of the heavy elements produced inthis process for various initial conditions.

Production of Heavy Elements During the Explosion of a Low-Mass Neutron Star in a Close Binary