Radiation magnetohydrodynamics simulations of Population III star formation during the epoch of reionization

Open Access

Fig. 8

Same as Figure 4, but for the z = 6 simulations without (top row) and with (bottom row) external radiation 200 yr after the formation of the first star. Note that the extent of the projection, and the color scales for temperature and number density differ from those in Figure 4.

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