Fig. 4
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Same as Fig. 3, but showing the dependence of the planet-induced gas flow on the Mach number of the headwind. We set m = 0.2 in all panels. The results were obtained from m02-hw0 (panel a), m02-hw001 (panel b), m02-hw003 (panel c), and m02-hw01 (panel d). The vertical dotted line corresponds to the corotation radius for the gas.
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