Studying the structure and kinematics of the gas in our simulations. Panels a–e display a set of azimuthally averaged quantities along the equatorial regions with respect to radius, where the equator was defined as the region where θ/π ∈ [0.45; 0.55] at a moment in time where the inner disk has reached ≈1 AU in radius. Panel a displays the density, panel b shows the radial velocity, panel c presents the azimuthal velocity, panel d shows the specific angular momentum, and panel e presents the temperature. Panel f displays the enclosed angular momentum profile. Panel g displays the deviation from Keplerian rotation along the disk midplane. Panel h displays the column density profile of the inner disk, where non-disk cells were masked.