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Caption: Figure 7.
Fraction of rpTDEs ﹩{f}_{\lt {T}_{{\rm{obt}}}}^{{\rm{Hills}}}({M}_{\bullet })﹩ as a function of SMBH mass for Tobt ∈ {1, 3, 10} yr contributed by binary disruptions and calculated from Equation (38), assuming that a fraction fb,hard = 20% of stars are in hard binaries.
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