Fig. 3.
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NGC 1052 stellar kinematics maps from our pPXF analysis (Sect. 3.2). These maps, velocity (left) and velocity dispersion (right), are displayed in units of km s−1. In both panels the large-scale kinematics are obtained from MUSE data, whereas the insets show the smoothed pPXF-maps from MEGARA datacube. The cross indicates the photometric centre as in Fig. 1.
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