Fraction of rpTDEs ﹩{f}_{\lt {T}_{{\rm{obt}}}}({M}_{\bullet })﹩ among all star disruptions as a function of SMBH mass for T_obt ∈ {1, 3, 10} yr obtained from Equations (15)–(18), where we have used β_rpTDE = 0.5. The blue and orange lines represent the fractional rates of rpTDEs from solar-type stars (1 M_⊙) and more massive stars (2 M_⊙), respectively.