Searching for intergalactic star forming regions in Stephan’s Quintet with SITELLE

Based on SITELLE spectroscopy, we studied the ionised gas emission for 175 H$\alpha$ regions in Stephan's Quintet (SQ). A detailed analysis is performed of star formation rate (SFR), oxygen abundance (O/H), and nitrogen-to-oxygen ratio (N/O) SQ regions, to explore provenance evolution this complex structure. According BPT diagram, found 91 HII, 17 composite, 7 active galactic nucleus-like SQ. Several are compatible with fast shocks models without a precursor solar metallicity low density (n=0.1 cm$^{-3}$), velocities between - 300 km s$^{-1}$. We derived total SFR (log(SFR/M$_\odot\,yr^{-1}$=0.496); starburst B provide 28% 9% SFR, 45% comes from radial velocity lower than 6160 For reason, assume that material prior collision new intruder (NI) does not show high therefore was apparently quenched. When considering integrated whole NI, both zones have consistent those obtained SDSS star-forming galaxies. At least two chemically different components cohabit where, average, (v$>$6160 s$^{-1}$) values O/H N/O (v$\leq$6160 s$^{-1}$). The line ratios, O/H, southern debris region northernmost tidal tail, belonging outer part highlight presence inner-outer variation some ratios along NI strands young tail south strand. Finally, outside galaxies because interactions dispersed peripheral zones.