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Fig. 1

image

Density slices perpendicular (first and second row, zoomed by a factor of 10) and parallel (third and fourth row, zoomed by a factor of 5) to the disk plane, at t ≈ 50 kyr. Streamlines corresponding to magnetic field lines and arrows corresponding to the velocity field are overplotted. Columns from left to right: Runs NOTURB, SUPA, SUPAS, and SUBA. The mass density ρ = 10−19 g cm−3 corresponds to the particle density n = 2.6 × 104 cm−3 and ρ = 10−11 g cm−3 to n = 2.6 × 1012 cm−3. White dots represent sink particles.

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