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The recently discovered burst of gravitational waves GW150914 provides a good new chance to verify the current view on the evolution of close binary stars. Modern population synthesis codes help to study this evolution from two main sequence stars up to the formation of two final remnant degenerate dwarfs, neutron stars or black holes. To study the evolution of the GW150914 predecessor we use the "Scenario Machine" code. The scenario modeling conducted in this study allowed to describe the evolution of systems for which the final stage is a massive BH+BH merger.