The Disc Miner - II. Revealing gas substructures and kinematic signatures from planet-disc interaction through line profile analysis

Open Access

Fig. B.19

As Fig. 14 but for the disc of GM Aur. The calculation of velocity profiles illustrated in this Figure excludes +45° wedges around the (north and south) disc minor axis to minimise contamination from infalling material (see Sect. 3.2, GM Aur).

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