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 $0.2 \rm{AU}$