Fig. 1.
Continuum (left) and Hα (right) emission maps of SDSS J143245.98+404300.3 obtained from the MaNGA data. The red dashed line highlights the position of the off-nuclear HII region where the high-velocity gas component has been found. The white cross indicates the photometric center of the galaxy. We have also highlighted in gray the two positions used for the long-slit spectroscopic observations with ISIS/WHT.
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