Title: Presentation of IFU data from MUSE for NGC 5291 N.

Abstract:
NGC 5291 N is a dwarf galaxy, formed in a huge HI ring that expanded in the intergalactic 
medium after a recent galaxy-galaxy collision. Undergoing a very recent starburst and showing 
evidences for the presence of Wolf-Rayet stars, NGC 5291 N stands out among Blue Compact 
Dwarf Galaxies because of its high, more than half-solar, metallicity, similar to that of tidal dwarf 
galaxies. I will present IFU data from MUSE that allow us to study precisely the physical 
properties of both the emission lines and the continuum, and to compare NGC 5291 N to other 
HII regions.