Fig. 9.
Maps of particle number density in log scale close to the stellar surface after about 60 h of evolution for runs FL-REF (upper panel), FL-HD (middle panel), and FL-LP (lower panel). The high-density regions (pointed at by white arrows) correspond to accretion columns impacting onto the stellar surface. Runs FL-REF and FL-HD exhibit clear hotspots, whereas in run FL-LF, the matter is more diffused and the contrast in density is weaker.
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