Massive Overflow Scenario

The initial conditions of the massive overflow scenario (MOS) is a 1 \rm{M}_{\odot} \thinspace \thinspace \thinspace \thinspace \thinspace \thinspace \thinspace \thinspace \thinspace \thinspace 1 \rm{R}_{\odot} star tidally disrupted by a 10 \rm{M}_{\odot}-10 \rm{M}_{\odot} black hole binary that has a separation of 0.2 \rm{AU}

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