My group studies all things eccentric (hover over image for names). We are particularly interested in relativistic stellar and gas dynamics near massive black holes, with applications to our Galactic center, the Andromeda (M31) nucleus and post-starburst galaxies. Some of us work on the dynamics of dark matter in disk galaxies and on globular clusters. We're also interested in the strange orbits of icy bodies in the outer solar system, and exoplanet dynamics!
The orbits of icy minor planets beyond Neptune are doing something very strange: they all tilt and pitch in similar ways, and maybe even cluster together on the sky. In a 2016 paper, my collaborator Mike McCourt and I show that when gravitational forces between minor planets on eccentric orbits are included in N-body simulations, the orbits incline rapidly off the disk plane, and tilt and pitch in exactly the same way.
The physics of how gas accretes onto supermassive black holes is hugely important in astrophysics. It is a difficult topic of research however, involving three-dimensional, hot, magnetic plasmas.
The double nucleus of the Andromeda galaxy has been a puzzle since its discovery by balloon-borne experiments in the early 1970s. It is best modeled as a single eccentric disk of stars, which orbits a massive black hole.
