Evolution of the cloud with an embedded binary, components of which become unbound via the three-body interaction at the pericentre passage near the central SMBH. The initial trajectory of the binary barycentre corresponds to the nominal trajectory of the G2/DSO (black solid line), whereas the post-pericentre stage depends strongly on the path of the individual components emerging from the system. Two exemplary cases are shown in different columns, corresponding to the choice of the component masses . Left panel: , . Right panel: , .