Fig. 2.

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Density maps for simulations A, B, C, and D. The plots represent the logarithmic density in PLUTO units (ρPLUTO = 2.48 × 10−15 g cm−3). The velocity vectors are shown through the black arrows, and the magnetic field lines are represented by the solid white lines. The distances on the vertical (z) and horizontal (ϖ) axis are represented in astronomical units. All the plots refer to PLUTO time = 100, which corresponds to approximately 12 stellar rotations.
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