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Hydrodynamical simulations show that the ram-pressure stripping in galaxyclusters fosters a strong interaction between stripped interstellar medium(ISM) and the surrounding medium, with the possibility of intracluster medium(ICM) cooling into cold gas clouds. Exploiting the MUSE observation of threejellyfish galaxies from the GAs Stripping Phenomena in galaxies with MUSE(GASP) survey, we explore the gas metallicity of star-forming clumps in theirgas tails. We find that the oxygen abundance of the stripped gas decreases as afunction of the distance from the parent galaxy disk; the observed metallicityprofiles indicate that more than 40% of the most metal-poor stripped clouds areconstituted by cooled ICM, in qualitative agreement with simulations thatpredict mixing between the metal-rich ISM and the metal-poor ICM.

Evidence for mixing between ICM and stripped ISM by the analysis of the gas metallicity in the tails of jellyfish galaxies