1 Introduction The standard picture of a tidal disruption event (TDE) involves the disruption of a star that enters the tidal sphere of a supermassive black hole (SMBH), which has a radius r t = R ⋆ M • / M ⋆ 1 / 3 $$ {r}_{\mathrm{t}}={R}_{\star }{\left({M}_{\bullet }/{M}_{\star}\right)}^{1/3} $$ (where R ⋆ $$ {R}_{\star } $$ is the stellar radius, and M ⋆ $$ {M}_{\star } $$ and M • $$ {M}_{\bullet } $$ are the stellar and SMBH masses, respectively), from a distance comparable to the sphere...