Fig. D.2.
Large-scale stellar kinematics of NGC 584 (MUSE), NGC 2784 (VIMOS), and NGC 7049 (VIMOS). Shown are the mean velocity V, velocity dispersion σ, and the h3 and h4 Hermite polynomials extracted by using pPXF. The data reduction and extraction of the kinematics are detailed described in Sect. 4.3. The image orientation is such that north is up and east is left.
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