Fig. A.5
(General comments about the panels as in Fig. A.1.) IRAS F05189-2524: this galaxy shows a compact Hα emission, both in the narrow and broad components.Their velocity fields and velocity dispersion maps do not show regular patterns. The broad component is blueshifted up to ~400 km s-1 with respect to the narrow one and is dominant in terms of flux in the innermost spaxels. The scale is of 0.839 kpc/′′.
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