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We investigated the star formation efficiency for all the dust emittingsources in Stephan's Quintet (SQ). We inferred star formation rates usingSpitzer MIR/FIR and GALEX FUV data and combined them with gas column densitymeasurements by various authors, in order to position each source in aKennicutt-Schmidt diagram. Our results show that the bright IGM star formationregions in SQ present star formation efficiencies consistent with thoseobserved within local galaxies. On the other hand, star formation in theintergalactic shock region seems to be rather inhibited.

The star formation efficiency in Stephan's Quintet intragroup regions