Fig. D.5.

nGC3 PCMs for a random realisation of particles in the rgal range 13–14 kpc, for each of the three warp models: Simple Symmetric warp (left), the Sine Lopsided warp (centre) and the S Lopsided warp (right). The colour scales linearly with star counts, indicating larger values with darker colours. Dotted circles and radial lines correspond respectively to parallels at co-latitudes increasing by 2° and meridians at azimuths every 30°.
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