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Fig. 12


Smoothed (σ = 1.3 pix) cut at z = 0.05 pc through the temperature cube of the simulation, with the black contours (N = 5 × 1021 cm−2) roughly indicating the high column density filament. Note the local increase in temperature at the sub-filament border due to the accretion shocks and the temperature drop in the sub-filaments after the shock compared to the inflowing mass reservoir. Because of smoothing, the temperature peaks of the shocked gas in the map have decreased. The area of the simulation that is covered by this figure is indicated in Fig. 11.

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