STELLAR AND GAS DYNAMICAL MODEL FOR TIDAL DISRUPTION EVENTS IN A QUIESCENT GALAXY
STELLAR AND GAS DYNAMICAL MODEL FOR TIDAL DISRUPTION EVENTS IN A QUIESCENT GALAXY
A detailed model of the tidal disruption events (TDEs) has been constructed using stellar dynamical and gas dynamical inputs that include black hole (BH) mass $M_{\bullet}$, specific orbital energy $E$ and angular momentum $J$, star mass $M_{\star}$ and radius $R_{\star}$, and the pericenter of the star orbit $r_{p}(E,\hspace{1mm}J,\hspace{1mm}M_{\bullet})$. We solved …