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\label{fig:MassiveIGWhist} Kippenhahn diagram of our stellar model shown in Figure \ref{fig:Massivestruc}, with the x-axis showing the time until core collaspe. Light blue shaded regions are convective. Solid colored lines show helium, carbon, oxygen, silicon, and iron core masses. Dashed vertical lines show the locations (from left) of our helium core burning, carbon shell burning, oxygen shell burning, and silicon shell burning models, respectively. The mass coordinate of the base of the convective shell, from which IGW propagate downwards, is labeled by a circle for each dashed line.