Kavli Affiliate: Mark Vogelsberger | Summary:We present a high-resolution hydrodynamical simulation of the formation and evolution of nuclear structures in a Milky Way-mass galaxy using the SMUGGLE multiphase ISM and stellar feedback model. The system naturally develops a bar of length $approx5$ kpc in isolation, driving sustained gas inflows toward the center that lead to […]
Continue.. SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk