Fig. 1.

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Density-weighted projections of the density along the z-axis with a physical width of 4000 au for halo 1 when reaching a peak density of 3 × 10−13 [g cm−3] using an initial magnetic field of B0 = 10−14 [G] (proper). From top to bottom the Jeans resolution was varied using 32, 64, 128, and 256 cells per Jeans length, and from left to right the strength of the radiation background was varied to J21 = 102, 103, 104, and 105. The halo shows more complex structures with increasing Jeans resolution as the turbulence seems to be better resolved. This occurs regardless of the value of J21.
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