Fig. A.14
(General comments about the panels as in Fig. A.1.) IRAS F07027-6011 (AM 0702-601): these maps correspond to the southern galaxy of the system. The velocity field of the narrow component is rather regular. In the velocity dispersion map a local maximum is found in correspondence of the nucleus (or Hα peak). The spatial scale is of 0.626 kpc/′′.
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