Simulations of layered protoplanetary disks find that rings form in the inner dead zone, migrate inward, and trigger FUor-like accretion events.
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Dynamical Gaseous Rings in Global Simulations of Protoplanetary Disk Formation
Simulations of layered protoplanetary disks find that rings form in the inner dead zone, migrate inward, and trigger FUor-like accretion events.