Illustration of the two planet-driven outflow regimes (based on Fendt (2003), Figure 1), showing a planet embedded in a circumstellar disk (CSD). (a) Jet: Outflows exceeding the escape velocity (v_w > v_e) escape the CPD. (b) Bipolar blob: Sub-escape-velocity outflows (v_w < v_e) remain gravitationally bound to the planet as it orbits. The bipolar blobs are reshaped (with respect to Fendt (2003)) to better match the observed structure of weak outflows in numerical models (e.g., Chrenko & Lambrechts 2019; Chrenko et al. 2025)