Title:
Mass segregation and TDEs in eccentric nuclear disks

Abstract:
The Andromeda galaxy contains a parsec scale eccentric disk. 
Secular torques can efficiently push stars in such disks to nearly radial orbits, 
where they can be tidally disrupted. In fact, a significant fraction of 
observed TDEs may come from these eccentric nuclear disks (ENDs). 
Previous work on these structures has considered disks with a single stellar population. 
I will discuss the dynamics of two-component ENDs. In particular, 
I will discuss how heavier stars in these disks mass segregate, 
and how this would increase their TDE rates.