MRI-active inner regions of protoplanetary discs. I. A detailed model of disc structure

no code implementations • 25 Feb 2021 • Marija R. Jankovic, James E. Owen, Subhanjoy Mohanty, Jonathan C. Tan

Here we present a steady-state model for inner discs accreting viscously, primarily due to the MRI.

Earth and Planetary Astrophysics Solar and Stellar Astrophysics