Three-temperature radiation hydrodynamics with PLUTO: Thermal and kinematic signatures of accreting protoplanets

Open Access

Fig. A.3

Sky-projected velocity perturbation, $υ_{⊥}^{'}$ $\upsilon _ \bot ^\prime$ , for a Jupiter-mass planet with no accretion luminosity. Relative to the fiducial case, circumplan-etary and in-gap flow patterns are significantly stronger.

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