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Fig. 2.

image

Upper panel: schematic sketch of the jet model, showing our geometric implementation of the three models. Lower panel: launching region and velocity field of the jet for the stellar jet (A), the disk wind (B), and the X-wind (C). Unlike the stellar jet and X-wind, the launching region for the disk wind is the region between the inner-disk radius din and the outer disk radius dout. This configuration is based on the disk wind configuration applied by Kurosawa et al. (2006).

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