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Fig. 3.

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Radial profiles of the magnetic, turbulent and thermal pressures for the no feedback runs at around t = 1 Gyr. Darker colors represents higher Jeans floor (NJ = (4, 8, 10, 16)). For the thermal pressure we only plot one line as it is similar across these simulations. For the NJ = 8 case we can see that the magnetic pressure is of similar strength as the thermal pressure in the center of the disk. The magnetic pressure decreases with radius and returns to initial values beyond 14 kpc. The turbulent pressure can be seen to significantly increases in both NJ = 4 and 8 as the disk is highly gravitationally unstable.

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