Fig. 3.

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Set of slices showing the evolution of the density (first two columns) and temperature (last two columns) for run IMHD (first and third columns, panels a–e and k–o) and run NIMHD (second and fourth columns, panels f–j and p–t). Each row represents a different time, where t = 0 corresponds to the moment of protostellar birth. For comparative purposes, the slices are shown at similar times, and the timestamp is written in the top right corner of each panel. The slices are done in the z direction for run IMHD, and along the angular momentum vector for run NIMHD. The scale bars in the first row apply to all the other rows as well.
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