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The Rossby wave instability (RWI) is a promising mechanism for producing large‐scale vortices in protoplanetary discs. The instability operates around a density bump in the disc, and the resulting vortices may facilitate planetesimal formation and angular momentum transfer in the disc dead zone. Most previous works on the RWI deal with 2D (height‐integrated) discs. However, vortices in 3D may have...
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